Influence of Obstructive Sleep Apnea on the Risk of Dental Caries: Insights from a 13-Year Population-Based Retrospective Study

KNOWLEDGE TRANSFER STATEMENT

Obstructive sleep apnea has been proven to have a great negative impact on patients, and the relationship between sleep apnea and dental caries is still inconclusive. Our study shows that patients with sleep apnea and those older than 45 y have a significant risk of dental caries.

Temporal Structures in Positron Spectra and Charge-Sign Effects in Galactic Cosmic Rays

We present the precision measurements of 11 years of daily cosmic positron fluxes in the rigidity range from 1.00 to 41.9 GV based on 3.4×10^{6} positrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The positron fluxes show distinctly different time variations from the electron fluxes at short and long timescales. A hysteresis between the electron fluxes and the positron fluxes is observed with a significance greater than 5σ at rigidities below 8.5 GV. On the contrary, the positron fluxes and the proton fluxes show similar time variation. Remarkably, we found that positron fluxes are modulated more than proton fluxes with a significance greater than 5σ for rigidities below 7 GV. These continuous daily positron fluxes, together with AMS daily electron, proton, and helium fluxes over an 11-year solar cycle, provide unique input to the understanding of both the charge-sign and mass dependencies of cosmic rays in the heliosphere.

Properties of Cosmic-Ray Sulfur and Determination of the Composition of Primary Cosmic-Ray Carbon, Neon, Magnesium, and Sulfur: Ten-Year Results from the Alpha Magnetic Spectrometer

We report the properties of primary cosmic-ray sulfur (S) in the rigidity range 2.15 GV to 3.0 TV based on 0.38×10^{6} sulfur nuclei collected by the Alpha Magnetic Spectrometer experiment (AMS). We observed that above 90 GV the rigidity dependence of the S flux is identical to the rigidity dependence of Ne-Mg-Si fluxes, which is different from the rigidity dependence of the He-C-O-Fe fluxes. We found that, similar to N, Na, and Al cosmic rays, over the entire rigidity range, the traditional primary cosmic rays S, Ne, Mg, and C all have sizeable secondary components, and the S, Ne, and Mg fluxes are well described by the weighted sum of the primary silicon flux and the secondary fluorine flux, and the C flux is well described by the weighted sum of the primary oxygen flux and the secondary boron flux. The primary and secondary contributions of the traditional primary cosmic-ray fluxes of C, Ne, Mg, and S (even Z elements) are distinctly different from the primary and secondary contributions of the N, Na, and Al (odd Z elements) fluxes. The abundance ratio at the source for S/Si is 0.167±0.006, for Ne/Si is 0.833±0.025, for Mg/Si is 0.994±0.029, and for C/O is 0.836±0.025. These values are determined independent of cosmic-ray propagation.

Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays

We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0×10^{8} electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations with periods of 27 days, 13.5 days, and 9 days are observed. We find that the electron fluxes show distinctly different time variations from the proton fluxes. Remarkably, a hysteresis between the electron flux and the proton flux is observed with a significance of greater than 6σ at rigidities below 8.5 GV. Furthermore, significant structures in the electron-proton hysteresis are observed corresponding to sharp structures in both fluxes. This continuous daily electron data provide unique input to the understanding of the charge sign dependence of cosmic rays over an 11-year solar cycle.

Modification of ERα by UFM1 Increases Its Stability and Transactivity for Breast Cancer Development

The post-translational modification (e.g., phosphorylation) of estrogen receptor α (ERα) plays a role in controlling the expression and subcellular localization of ERα as well as its sensitivity to hormone response. Here, we show that ERα is also modified by UFM1 and this modification (ufmylation) plays a crucial role in promoting the stability and transactivity of ERα, which in turn promotes breast cancer development. The elevation of ufmylation via the knockdown of UFSP2 (the UFM1-deconjugating enzyme in humans) dramatically increases ERα stability by inhibiting ubiquitination. In contrast, ERα stability is decreased by the prevention of ufmylation via the silencing of UBA5 (the UFM1-activating E1 enzyme). Lys171 and Lys180 of ERα were identified as the major UFM1 acceptor sites, and the replacement of both Lys residues by Arg (2KR mutation) markedly reduced ERα stability. Moreover, the 2KR mutation abrogated the 17β-estradiol-induced transactivity of ERα and the expression of its downstream target genes, including pS2, cyclin D1, and c-Myc; this indicates that ERα ufmylation is required for its transactivation function. In addition, the 2KR mutation prevented anchorage-independent colony formation by MCF7 cells. Most notably, the expression of UFM1 and its conjugating machinery (i.e., UBA5, UFC1, UFL1, and UFBP1) were dramatically upregulated in ERα-positive breast cancer cell lines and tissues. Collectively, these findings implicate a critical role attributed to ERα ufmylation in breast cancer development by ameliorating its stability and transactivity.

Properties of Daily Helium Fluxes

We present the precision measurement of 2824 daily helium fluxes in cosmic rays from May 20, 2011 to October 29, 2019 in the rigidity interval from 1.71 to 100 GV based on 7.6×10^{8} helium nuclei collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The helium flux and the helium to proton flux ratio exhibit variations on multiple timescales. In nearly all the time intervals from 2014 to 2018, we observed recurrent helium flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. In the entire time period, we found that below ∼7  GV the helium flux exhibits larger time variations than the proton flux, and above ∼7  GV the helium to proton flux ratio is time independent. Remarkably, below 2.4 GV a hysteresis between the helium to proton flux ratio and the helium flux was observed at greater than the 7σ level. This shows that at low rigidity the modulation of the helium to proton flux ratio is different before and after the solar maximum in 2014.

Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV

We present the precision measurement of the daily proton fluxes in cosmic rays from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV based on 5.5×10^{9} protons collected with the Alpha Magnetic Spectrometer aboard the International Space Station. The proton fluxes exhibit variations on multiple timescales. From 2014 to 2018, we observed recurrent flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. The rigidity dependence of the 27-day periodicity is different from the rigidity dependences of 9-day and 13.5-day periods. Unexpectedly, the strength of 9-day and 13.5-day periodicities increases with increasing rigidities up to ∼10  GV and ∼20  GV, respectively. Then the strength of the periodicities decreases with increasing rigidity up to 100 GV.

Erratum: Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen [Phys. Rev. Lett. 127, 021101 (2021)]

This corrects the article DOI: 10.1103/PhysRevLett.127.021101.

Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen

We report the properties of sodium (Na) and aluminum (Al) cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on 0.46 million sodium and 0.51 million aluminum nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We found that Na and Al, together with nitrogen (N), belong to a distinct cosmic ray group. In this group, we observe that, similar to the N flux, both the Na flux and Al flux are well described by the sums of a primary cosmic ray component (proportional to the silicon flux) and a secondary cosmic ray component (proportional to the fluorine flux). The fraction of the primary component increases with rigidity for the N, Na, and Al fluxes and becomes dominant at the highest rigidities. The Na/Si and Al/Si abundance ratios at the source, 0.036±0.003 for Na/Si and 0.103±0.004 for Al/Si, are determined independent of cosmic ray propagation.

Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer

Precise knowledge of the charge and rigidity dependence of the secondary cosmic ray fluxes and the secondary-to-primary flux ratios is essential in the understanding of cosmic ray propagation. We report the properties of heavy secondary cosmic ray fluorine F in the rigidity R range 2.15 GV to 2.9 TV based on 0.29 million events collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The fluorine spectrum deviates from a single power law above 200 GV. The heavier secondary-to-primary F/Si flux ratio rigidity dependence is distinctly different from the lighter B/O (or B/C) rigidity dependence. In particular, above 10 GV, the F/Si/B/O ratio can be described by a power law R^{δ} with δ=0.052±0.007. This shows that the propagation properties of heavy cosmic rays, from F to Si, are different from those of light cosmic rays, from He to O, and that the secondary cosmic rays have two classes.

Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer

We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×10^{6} iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.

Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer

We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8×10^{6}  Ne, 2.2×10^{6}  Mg, and 1.6×10^{6}  Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.

Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer

Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of ^{3}He and ^{4}He fluxes are presented. The measurements are based on 100 million ^{4}He nuclei in the rigidity range from 2.1 to 21 GV and 18 million ^{3}He from 1.9 to 15 GV collected from May 2011 to November 2017. We observed that the ^{3}He and ^{4}He fluxes exhibit nearly identical variations with time. The relative magnitude of the variations decreases with increasing rigidity. The rigidity dependence of the ^{3}He/^{4}He flux ratio is measured for the first time. Below 4 GV, the ^{3}He/^{4}He flux ratio was found to have a significant long-term time dependence. Above 4 GV, the ^{3}He/^{4}He flux ratio was found to be time independent, and its rigidity dependence is well described by a single power law ∝R^{Δ} with Δ=-0.294±0.004. Unexpectedly, this value is in agreement with the B/O and B/C spectral indices at high energies.

Towards Understanding the Origin of Cosmic-Ray Electrons

Precision results on cosmic-ray electrons are presented in the energy range from 0.5 GeV to 1.4 TeV based on 28.1×10^{6} electrons collected by the Alpha Magnetic Spectrometer on the International Space Station. In the entire energy range the electron and positron spectra have distinctly different magnitudes and energy dependences. The electron flux exhibits a significant excess starting from 42.1_{-5.2}^{+5.4}  GeV compared to the lower energy trends, but the nature of this excess is different from the positron flux excess above 25.2±1.8  GeV. Contrary to the positron flux, which has an exponential energy cutoff of 810_{-180}^{+310}  GeV, at the 5σ level the electron flux does not have an energy cutoff below 1.9 TeV. In the entire energy range the electron flux is well described by the sum of two power law components. The different behavior of the cosmic-ray electrons and positrons measured by the Alpha Magnetic Spectrometer is clear evidence that most high energy electrons originate from different sources than high energy positrons.

Towards Understanding the Origin of Cosmic-Ray Positrons

Precision measurements of cosmic ray positrons are presented up to 1 TeV based on 1.9 million positrons collected by the Alpha Magnetic Spectrometer on the International Space Station. The positron flux exhibits complex energy dependence. Its distinctive properties are (a) a significant excess starting from 25.2±1.8  GeV compared to the lower-energy, power-law trend, (b) a sharp dropoff above 284_{-64}^{+91}  GeV, (c) in the entire energy range the positron flux is well described by the sum of a term associated with the positrons produced in the collision of cosmic rays, which dominates at low energies, and a new source term of positrons, which dominates at high energies, and (d) a finite energy cutoff of the source term of E_{s}=810_{-180}^{+310}  GeV is established with a significance of more than 4σ. These experimental data on cosmic ray positrons show that, at high energies, they predominantly originate either from dark matter annihilation or from other astrophysical sources.

Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station

We present high-statistics, precision measurements of the detailed time and energy dependence of the primary cosmic-ray electron flux and positron flux over 79 Bartels rotations from May 2011 to May 2017 in the energy range from 1 to 50 GeV. For the first time, the charge-sign dependent modulation during solar maximum has been investigated in detail by leptons alone. Based on 23.5×10^{6} events, we report the observation of short-term structures on the timescale of months coincident in both the electron flux and the positron flux. These structures are not visible in the e^{+}/e^{-} flux ratio. The precision measurements across the solar polarity reversal show that the ratio exhibits a smooth transition over 830±30 days from one value to another. The midpoint of the transition shows an energy dependent delay relative to the reversal and changes by 260±30 days from 1 to 6 GeV.

Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station

A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to 3.3 TV based on 2.2×10^{6} events is presented. The detailed rigidity dependence of the nitrogen flux spectral index is presented for the first time. The spectral index rapidly hardens at high rigidities and becomes identical to the spectral indices of primary He, C, and O cosmic rays above ∼700  GV. We observed that the nitrogen flux Φ_{N} can be presented as the sum of its primary component Φ_{N}^{P} and secondary component Φ_{N}^{S}, Φ_{N}=Φ_{N}^{P}+Φ_{N}^{S}, and we found Φ_{N} is well described by the weighted sum of the oxygen flux Φ_{O} (primary cosmic rays) and the boron flux Φ_{B} (secondary cosmic rays), with Φ_{N}^{P}=(0.090±0.002)×Φ_{O} and Φ_{N}^{S}=(0.62±0.02)×Φ_{B} over the entire rigidity range. This corresponds to a change of the contribution of the secondary cosmic ray component in the nitrogen flux from 70% at a few GV to <30% above 1 TV.

Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station

We present the precision measurement from May 2011 to May 2017 (79 Bartels rotations) of the proton fluxes at rigidities from 1 to 60 GV and the helium fluxes from 1.9 to 60 GV based on a total of 1×10^{9} events collected with the Alpha Magnetic Spectrometer aboard the International Space Station. This measurement is in solar cycle 24, which has the solar maximum in April 2014. We observed that, below 40 GV, the proton flux and the helium flux show nearly identical fine structures in both time and relative amplitude. The amplitudes of the flux structures decrease with increasing rigidity and vanish above 40 GV. The amplitudes of the structures are reduced during the time period, which started one year after solar maximum, when the proton and helium fluxes steadily increase. Above ∼3  GV the p/He flux ratio is time independent. We observed that below ∼3  GV the ratio has a long-term decrease coinciding with the period during which the fluxes start to rise.

Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station

We report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4×10^{6} nuclei collected by AMS during the first five years of operation aboard the International Space Station. The Li and B fluxes have an identical rigidity dependence above 7 GV and all three fluxes have an identical rigidity dependence above 30 GV with the Li/Be flux ratio of 2.0±0.1. The three fluxes deviate from a single power law above 200 GV in an identical way. This behavior of secondary cosmic rays has also been observed in the AMS measurement of primary cosmic rays He, C, and O but the rigidity dependences of primary cosmic rays and of secondary cosmic rays are distinctly different. In particular, above 200 GV, the secondary cosmic rays harden more than the primary cosmic rays.

Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station

We report the observation of new properties of primary cosmic rays He, C, and O measured in the rigidity (momentum/charge) range 2 GV to 3 TV with 90×10^{6} helium, 8.4×10^{6} carbon, and 7.0×10^{6} oxygen nuclei collected by the Alpha Magnetic Spectrometer (AMS) during the first five years of operation. Above 60 GV, these three spectra have identical rigidity dependence. They all deviate from a single power law above 200 GV and harden in an identical way.

A Case of Persistent and Recurrent Ventricular Fibrillation with Successful Resuscitation and Good Neurological Outcome

A 49-year-old man suffering from chest pain collapsed on arrival at an emergency department. Ventricular fibrillation was confirmed and he survived neurologically normal after 22 defibrillation shocks. This case attests that persistent and recurrent ventricular fibrillation is still compatible with good neurological outcome. Energetic and persistent efforts should be continued in such cases. Amiodarone should be considered early in the course of refractory ventricular fibrillation.

An Analysis of Unscheduled Return Visits to the Accident and Emergency Department of a General Public Hospital

Objectives

To identify the reasons for unscheduled return visits to a public emergency department and possible strategies to reduce unscheduled return visits.

Design

Cross-sectional survey.

Setting

A public emergency department in Hong Kong.

Patients

Unscheduled return visits within 48 hours in a three-month period from 14 January 2000 to 15 April 2000.

Main outcome measures

Patients' epidemiological characteristics, reasons, complaints and outcome of the unscheduled return visits.

Results

During the study period, 3.3% (1,060) of the attendance was unscheduled return visits within 48 hours as recorded in the computerized A&E Information System of the hospital. However, only 738 patients (70%) responded to the questionnaire. These 738 patients formed the study population for further analysis. Illness-related factors accounted for 87% of the total unscheduled return visits. Patient-related factors were responsible for about 10% of unscheduled return visits. Doctor-related factors accounted for about 3% of unscheduled return visits. There was only one system-related unscheduled return visit. For the outcome of return visits, about 76% (559) was discharged after the second consultation. About 5% (40) was referred to specialist clinics. Around 24% (179) of patients was admitted. Of those admitted, 78% (140) was illness-related, 13% (23) was patient-related and 9% (16) was doctor-related. Upper respiratory tract infection was the most frequent complaint (34%), followed by painful conditions (23%) and injuries (10%). For children at or below 10 years of age, upper respiratory tract infection (60%) and febrile illness (15%) were the most frequent complaints.

Conclusions

The study found that the reasons for return visits were multiple. These “unscheduled return visits” should not be automatically regarded as poor indicator of service. Better patient education, organized family practice system, upgrading of professional training and targeted audit are possible means to reduce unscheduled return visits.

Go-Kart Related Injuries: A Local Scene

Objectives

To study the characteristics and nature of injuries relating to go-kart in the local setting and to compare the findings with those reported in the medical literature.

Methods

A prospective survey of patients with go-kart related injuries attending the accident and emergency department of a public district hospital in Hong Kong within the year 2002. The data were analysed and compared with previous studies.

Results

Forty-two patients were collected in the study. The mean age was 26 years. Ten patients (23.8%) were at or below the age of 20 years. Twenty-nine patients (69.0%) were males. Out of the 42 patients, all were riders except one who was a bystander. Thirty-three patients (78.6%) had injuries in indoor tracks. Ten (23.8%) patients were admitted and five (50%) of those admitted required operations. There was no fatality. Twenty-seven patients (64.3%) had only single injury. Most (64.2%) were minor soft tissue injuries. However, fractures or dislocations occurred in 13 patients (31.0%). Two patients (4.8%) suffered from internal organ injuries. Isolated head and facial injuries occurred in 11.9% of patients. All were simple concussion. Nine patients (21.4%) suffered from isolated lower limb injuries, with more than half sustaining fractures or dislocations. Collision with other karts (40.5%) was the most frequent mechanism of injury. Riding in outdoor track was associated significantly with increased admission when compared with indoor track (77.8% vs 9.1%, p<0.001). There was no association between rider's age, gender, previous riding or injury experience, or the presence of briefing before the race with the rate of admission.

Conclusion

Go-kart racing and working on racing track can be a recreation or occupation with potential dangers. In our study, characteristics of patients, mechanisms and types of injuries were similar to other western studies. Accidents on outdoor tracks appeared to be more serious and more likely admitted than those on indoor circuits. Special safety precautions on outdoor events may help to reduce the severity of injuries. However, drivers with more riding or injury experiences were not exempted from severe injuries. Moreover, presence of briefing before the race did not help reduce the admission rate either. Perhaps, a safe and careful attitude of the rider and a seriously conducted briefing by a qualified instructor would be more important to reduce accidents. Further proper large scale controlled epidemiological studies will definitely help to improve the understanding of go-kart related injuries.

Pancreatic Injury: An Uncommon Cause of Abdominal Pain after Blunt Trauma

Blunt pancreatic injury is an uncommon cause of traumatic abdominal pain. Early diagnosis is difficult due to its subtle initial presentation, both clinically and on imaging study. Dilemma between a watchful expectant management and thorough initial investigation may arise. The management of a 44-year-old man presenting to the emergency department because of generalised trunk pain after blunt trauma is reported.

Golf-related Injuries: Case Series and Reports

Within the year 2002, eleven patients attended the emergency department of a public district hospital because of golf-related injuries. This attested to the low but occasionally serious risk of this type of sport activity. As golf is becoming increasingly popular in Hong Kong, it is expected that emergency physicians will see more and more golf-related injuries.

Acute Ischaemic Stroke: Management, Recent Advances and Controversies

Acute ischaemic stroke is a major cause of death and disability. It may become an enormous burden to the patients themselves, their families as well as the health care systems. Patients at risk of airway, breathing and circulatory compromise should receive prompt resuscitation. Vital parameters and neurological status should be closely monitored. Attentions to blood pressure, temperature and sugar profile are important. The significance of early and correct diagnosis and subsequent treatment cannot be over-emphasised. There have been tremendous recent advances in different treatment modalities in acute stroke management. Various recanalisation modalities include intravenous and/or intra-arterial thrombolysis, acute defibrinogenation, anti-platelet treatment and anticoagulation. Carotid endarterectomy and endovascular strategies are recommended in selected patients. Advanced neuro-imaging techniques and neuroprotectants are being evaluated. Multidisciplinary stroke teams have been shown to improve patient survival and functional outcome. Pre-defined algorithms and protocols should be in place to expedite smooth and effective delivery of stroke service. Future directions should be aimed at exploring safer recanalisation modalities and extending the limit of the current 3-hour treatment window for thrombolysis.

A Retrospective Study of Seclusion in an Emergency Department

Objectives

To study the practice of seclusion in an emergency department (ED) and to explore high-risk elements during seclusion.

Methods

The study consisted of two parts: an in-depth analysis on all incidents associated with seclusion in a six-year period (1998–2004) and a two-year (2002–2004) retrospective analysis of secluded patient records to understand the rationale and patient outcome.

Results

Part 1: A total of 9 incident records were collected. Four patients were related to setting fire. Five patients had violence or threat of violence. The median length of stay (LOS) in seclusion at the time of incident was 129 minutes. Although 66.7% of the patients had additional restraint prior to the seclusion, incidents still occurred. Two staff sustained injuries and hospital facilities were damaged in some of the incidents. Six patients were later admitted to psychiatric hospital. Part 2: 141 patient data were collected in the study (M: 89 and F: 52). The average monthly number of patients secluded was about 6. The mean age was 45 years (SD 19) and the mean LOS was 616 minutes (SD 478). There were three incidences (2.1%) during the two-year period. A total of 82 patients (58.2%) were associated with violence or threat of violence and 38 (46.3%) of the group had psychiatric illness; and 50 patients (35.5%) were associated with alcohol or drug intoxication. Ultimately, 56 patients (39.7%) were admitted to psychiatric hospital and 64 patients (45.4%) were treated and discharged from the ED.

Conclusion

Seclusion is a high-risk practice. In our department, the most frequent indication was violence (58.2%), with nearly half of them having history of psychiatric illness. Psychiatric illness had the highest risk for incidents, especially those with violence or threat of violence. The LOS in seclusion was relatively long in the ED and might be one of the risk factors for incidents. Inadequate removal of potentially dangerous belongings from patients before seclusion may end up with catastrophic outcomes. Curiously, ED nurses are not allowed to search patients before seclusion. They are exposed to legal liability in exercising restraint and in searching for potentially dangerous items from patients. It is suggested that clear protocols and quality assurance programs should be instituted to ensure safe seclusion.

Prognostic Predictive Values of the Initial Electrocardiogram with St-Segment Elevation Acute Myocardial Infarction in Chinese Patients

Objective

To study the electrocardiogram (ECG) features that predict 30-day mortality of ST-segment elevation acute myocardial infarction (STEMI) in Chinese patients.

Method

This was a retrospective study. Patients presenting within twelve hours after the onset of chest pain with ECG features compatible with STEMI and the diagnosis confirmed after admission were included in the study. Data taken into account included age, sex and thrombolytic therapy in the emergency department. The hospital records of the patients were later retrieved from the computer. The initial ECG performed in the emergency department were reviewed.

Results

A total of 98 patients were included in the study. There was no statistically significant relationship between 30-day mortality and the type of myocardial infarction or the magnitude of the ST segment changes. Distortion of the terminal portion of the QRS complex and prior evidence of myocardial infarction (in another location different from the presenting one) showed statistically significant relationship with 30-day mortality, with odds ratio 10.364 (95% CI 1.715–62.620) and 12.731 (95% CI 2.317–69.962) respectively.

Conclusion

In newly diagnosed STEMI patients, if there is evidence of terminal distortion of the QRS complex or prior ECG changes of myocardial infarction, the 30-day mortality will be significantly higher.

A Lady with Alarming Neck Swelling after Minor Head Injury

A 52-year-old woman with hidden ankylosing spondylitis for years attended the emergency department after a minor head injury. Rapid and alarming neck swelling appeared shortly after the initial consultation. Although the physical examination and the lateral cervical spine X-ray did not suggest fracture, a later CT scan revealed a fracture line. A high index of suspicion and early use of the halo device are needed in order to prevent irreversible neurological damage in such patients.

Emergency Department Violence: a Local Scene

Objectives

To study the nature, frequency and magnitude of violence in a local emergency department.

Design

Prospective epidemiological study in a three-month period, during which involved staff filled in a survey form immediately after violence incidents.

Setting

Accident & Emergency Department of a public general hospital in the northeastern New Territories.

Population

Assailants and victims of violence in the emergency department.

Main outcome measures

Nature of violence, frequency, cause, morbidity, epidemiological characteristics of assailants and victims.

Results

There were 25 incidents with 26 assailants in the three-month period. The great majority was verbal abuse only (64%). No weapon was involved. Long waiting time (36%), deranged mental condition (28%) and dissatisfaction with service (20%) were the leading causes of violence. Assailants showed a predominance of male (69%) and age between 21–50 years. They were either patients (69%) or accompanying persons (31%). Nurses (59%) and to a lesser extent doctors (23%), were the main victims.

Conclusion

The incidence of emergency department violence (0.08%) was low and the majority was verbal abuse only. Nurses bore the brunt of the violence. Long waiting time, confused patients and dissatisfied patients were high risk factors.

Meeting the Media: Friend or Foe?

For various reasons, the emergency department is an area of interest for the media. As a result, emergency physicians have to prepare for the occasions of being interviewed by the media some day in their career. It is natural to have some anxiety and fear in meeting the media, especially for the inexperienced. However, developing a good relationship with the media would not only benefit the organisation and the specialty, but also the general public as well. This is a review of the preparation, techniques, tricks and pitfalls in dealing with the media, especially in regard to television interviews.

Ciguatera fish Poisoning: a Challenge to Emergency Physicians

Seven patients from two families presented with ciguatera poisoning after fish consumption. They suffered most of the typical clinical features of ciguatera poisoning and were given supportive treatments. Three of them were given mannitol infusion and showed improvement in symptoms. All of them were discharged within two days.

An Intravenous Drug Addict Presenting with ‘Shortness of Breath’: Case Report

A 49-year-old male intravenous drug addict attended the emergency department complaining of ‘shortness of breath’ for one day. He was discharged after evaluation and referred to the methadone clinic. He re-attended the next day complaining of neck stiffness and twitching of limbs for one day. The final diagnosis was tetanus. Although tetanus is rare in Hong Kong, high vigilance should still be maintained for its atypical presentations, especially in high-risk groups.

Alarming Pneumomediastinum but Benign Outcome: a Case Report on Oesophageal Perforation by Foreign Body

A case of oesophageal perforation after endoscopic removal of foreign body is described. A 50-year-old female had a sharp fish bone impacted in the cervical oesophagus. After dislodging the bone at endoscopy, she developed neck pain and swelling. Chest X-ray showed alarming pneumomediastinum and subcutaneous emphysema. However, there was no leakage in the water-soluble contrast swallow. She was successfully managed conservatively. Early recognition and proper management of such a well-known complication are important to lower morbidity, especially in view of the fact that endoscopic removal of swallowed foreign bodies is being performed on an outpatient basis in some emergency departments. Special precaution should be given to sharp foreign bodies lodged at the cervical oesophagus.

Delayed Rupture of Occult Splenic Injury: a Case Report

We report on a case of splenic rupture that presented eleven days after a trivial injury. Possible explanations of the delay in presentation and ways for early detection are discussed. Emergency physicians should always bear this entity in mind before discharging patients with left thoracoabdominal injury.