Development of a Pharmacy Point-of-Dispensing Toolkit for Anthrax Post-Exposure Prophylaxis for Allegheny County Postal Workers.

CONTEXT: The Centers for Disease Control and Prevention (CDC) and the US Postal Service (USPS) consider anthrax to be a potential threat to USPS workers. A county health department-owned pharmacy supports local USPS response in the event of an exposure. The pharmacy team identified the need to review and update the local anthrax response plan. PROGRAM/POLICY: A Pharmacy Point-of-Dispensing Toolkit and response plan for initial 10-day post-exposure antibiotic prophylaxis was developed for use by a local health department in the event of a mass anthrax exposure at a US Post Office sorting facility. The pharmacist's role in medical countermeasures planning for anthrax exposure is also discussed to illustrate how pharmacists' medication expertise can be utilized. EVALUATION: The CDC's Public Health Preparedness Capabilities: National Standards for State and Local Planning framework and inputs from an interprofessional stakeholder team were used to develop a Medical Countermeasures Response Plan and Implementation Toolkit for mass point-of-dispensing (POD) in the event of an anthrax exposure. IMPLEMENTATION AND DISSEMINATION: Stakeholders attended a USPS Community Partner Training event where additional revisions to the toolkit were made. The toolkit and standing order are now implemented at the local health department to be reviewed and updated on a yearly basis by health department leadership. DISCUSSION: Pharmacists can use their medication expertise and experience with patient education to design emergency response plans focused on increasing patient safety and medication adherence. Pharmacists should be involved in emergency response and medical countermeasures planning that involve medications.

Kinetic Study of the Reactions PO + O2 and PO2 + O3 and Spectroscopy of the PO Radical.

The kinetics of the reactions of PO with O2 and PO2 with O3 were studied at temperatures ranging from ∼190 to 340 K, using a pulsed laser photolysis-laser induced fluorescence technique. For the reaction of PO + O2, there is evidence of both a two- and three-body exit channel, producing PO2 + O and PO3, respectively. Potential energy surfaces of both the PO + O2 and PO2 + O3 systems were calculated using electronic structure theory and combined with RRKM calculations to explain the observed pressure and temperature dependences. For PO + O2, at pressures typical of a planetary upper atmosphere where meteoric ablation of P will occur, the reaction is effectively pressure independent with a yield of PO2 + O of >99%; the rate coefficient can be expressed by log10(k, 120-500 K, cm3 molecule-1 s-1) = -13.915 + 2.470 log10(T) - 0.5020(log10(T))2, with an uncertainty of ±10% over the experimental temperature range (191-339 K). With increasing pressure, the yield of PO3 increases, reaching ∼90% at a pressure of 1 atm and T = 300 K. For PO2 + O3, k(188-339 K) = 3.7 × 10-11 exp(-1131/T) cm3 molecule-1 s-1, with an uncertainty of ±26% over the stated temperature range. Laser-induced fluorescence spectra of PO over the wavelength range 245-248 nm were collected and simulated using pgopher to obtain new spectroscopic constants for the ground and v = 1 vibrational levels of the X2Π and A2Σ+ states of PO.

A study of the reactions of Ni+ and NiO+ ions relevant to planetary upper atmospheres.

The reactions between Ni+(2D) and O3, O2, N2, CO2 and H2O were studied at 294 K using the pulsed laser ablation at 532 nm of a nickel metal target in a fast flow tube, with mass spectrometric detection of Ni+ and NiO+. The rate coefficient for the reaction of Ni+ with O3 is k(294 K) = (9.7 ± 2.1) × 10-10 cm3 molecule-1 s-1; the reaction proceeds at the ion-permanent dipole enhanced Langevin capture rate with a predicted T-0.16 dependence. Electronic structure theory calculations were combined with Rice-Ramsperger-Kassel-Markus theory to extrapolate the measured recombination rate coefficients to the temperature and pressure conditions of planetary upper atmospheres. The following low-pressure limiting rate coefficients were obtained for T = 120-400 K and He bath gas (in cm6 molecule-2 s-1, uncertainty ±σ at 180 K): log10(k, Ni+ + N2) = -27.5009 + 1.0667log10(T) - 0.74741(log10(T))2, σ = 29%; log10(k, Ni+ + O2) = -27.8098 + 1.3065log10(T) - 0.81136(log10(T))2, σ = 32%; log10(k, Ni+ + CO2) = -29.805 + 4.2282log10(T) - 1.4303(log10(T))2, σ = 28%; log10(k, Ni+ + H2O) = -24.318 + 0.20448log10(T) - 0.66676(log10(T))2, σ = 28%). Other rate coefficients measured (at 294 K, in cm3 molecule-1 s-1) were: k(NiO+ + O) = (1.7 ± 1.2) × 10-10; k(NiO+ + CO) = (7.4 ± 1.3) × 10-11; k(NiO+ + O3) = (2.7 ± 1.0) × 10-10 with (29 ± 21)% forming Ni+ as opposed to NiO2+; k(NiO2+ + O3) = (2.9 ± 1.4) × 10-10, with (16 ± 9)% forming NiO+ as opposed to ONiO2+; and k(Ni+·N2 + O) = (7 ± 4) × 10-12. The chemistry of Ni+ and NiO+ in the upper atmospheres of Earth and Mars is then discussed.

Experimental Study of the Removal of Ground- and Excited-State Phosphorus Atoms by Atmospherically Relevant Species.

The reaction kinetics of the ground and first two excited states of atomic phosphorus, P, with atmospherically relevant species were studied at temperatures ranging from ∼200 to 750 K using a pulsed laser photolysis-laser-induced fluorescence technique. The temperature dependence of the rate coefficients is parametrized as follows (units: cm3 molecule-1 s-1, 1σ errors): k(P(2P)+O2)(189 ≤ T/K ≤ 701) = (7.10 ± 1.03) × 10-12 × (T/298)1.42±0.13 × exp[(374 ± 41)/T]; k(P(2D)+O2)(188 ≤ T/K ≤ 714) = (1.20 ± 0.29) × 10-11 × (T/298)0.821±0.207 × exp[(177 ± 70)/T]; k(P(2D)+CO2)(296 ≤ T/K ≤ 748) = (5.68 ± 0.36) × 10-12 × (T/298)0.800±0.103; k(P(2D)+N2)(188 ≤ T/K ≤ 748) = (1.42 ± 0.03) × 10-12 × (T/298)1.36±0.04; k(P(4S)+O2)(187 ≤ T/K ≤ 732) = (3.08 ± 0.31) × 10-13 × (T/298)2.24±0.29. Electronic structure theory combined with RRKM calculations have been used to explain the unusual temperature dependence of P(4S) + O2. The small pre-exponential factor for the reaction results from a tight steric constraint, together with the requirement that the reaction occurs on doublet rather than sextet electronic surfaces.

Kinetic Study of Ni and NiO Reactions Pertinent to the Earth's Upper Atmosphere.

Nickel atoms are injected into the Earth's mesosphere by meteoric ablation, producing a Ni layer between 70 and 105 km in altitude. The subsequent reactions of Ni and NiO with atmospherically relevant species were studied using the time-resolved pulsed laser photolysis-laser-induced fluorescence technique, combined with electronic structure calculations and RRKM theory where appropriate. Results for bimolecular reactions (in cm3 molecule-1 s-1): k(Ni + O3, 293 K) = (6.5 ± 0.7) × 10-10; k(NiO + O3 → Ni + 2O2, 293 K) = (1.4 ± 0.5) × 10-10; k(NiO + O3 → NiO2 + O2, 293 K) = (2.5 ± 0.7) × 10-10; k(NiO + CO, 190-377 K) = (3.2 ± 0.6) × 10-11 ( T/200)-0.19±0.05. For termolecular reactions (in cm6 molecule-2 s-1, uncertainty ± σ over the stated temperature range): log10( krec,0(Ni + O2 + N2, 190-455 K)) = -37.592 + 7.168log10( T) - 1.5650(log10( T))2, σ = 11%; log10( krec,0(NiO + O2 + N2, 293-380 K)) = -41.0913 + 10.1064log10( T) - 2.2610(log10( T))2, σ = 22%; and log10( krec,0(NiO + CO2 + N2, 191-375 K)) = -41.4265 + 10.9640log10( T) - 2.5287(log10( T))2, σ = 15%. The faster recombination reaction NiO + H2O + N2, which is clearly in the falloff region over the experimental pressure range (3-10 Torr), is best described by log10( krec,0/cm6 molecule-2 s-1) = -29.7651 + 5.2064log10( T) - 1.7118(log10( T))2, krec,∞ = 6.0 × 10-10 exp(-171/ T) cm3 molecule-1 s-1, broadening factor Fc = 0.84, σ = 16%. The implications of these results in the atmosphere are then discussed.

Upregulation of the coagulation factor VII gene during glucose deprivation is mediated by activating transcription factor 4.

BACKGROUND: Constitutive production of blood coagulation proteins by hepatocytes is necessary for hemostasis. Stressful conditions trigger adaptive cellular responses and delay processing of most proteins, potentially affecting plasma levels of proteins secreted exclusively by hepatocytes. We examined the effect of glucose deprivation on expression of coagulation proteins by the human hepatoma cell line, HepG2. METHODOLOGY/PRINCIPAL FINDINGS: Expression of coagulation factor VII, which is required for initiation of blood coagulation, was elevated by glucose deprivation, while expression of other coagulation proteins decreased. Realtime PCR and ELISA demonstrated that the relative percentage expression +/- SD of steady-state F7 mRNA and secreted factor VII antigen were significantly increased (from 100+/-15% to 188+/-27% and 100+/-8.8% to 176.3+/-17.3% respectively, p<0.001) at 24 hr of treatment. The integrated stress response was induced, as indicated by upregulation of transcription factor ATF4 and of additional stress-responsive genes. Small interfering RNAs directed against ATF4 potently reduced basal F7 expression, and prevented F7 upregulation by glucose deprivation. The response of the endogenous F7 gene was replicated in reporter gene assays, which further indicated that ATF4 effects were mediated via interaction with an amino acid response element in the F7 promoter. CONCLUSIONS/SIGNIFICANCE: Our data indicated that glucose deprivation enhanced F7 expression in a mechanism reliant on prior ATF4 upregulation primarily due to increased transcription from the ATF4 gene. Of five coagulation protein genes examined, only F7 was upregulated, suggesting that its functions may be important in a systemic response to glucose deprivation stress.