Gamma Ray Glow Observations at 20-km Altitude.

In the spring of 2017 an ER-2 aircraft campaign was undertaken over continental United States to observe energetic radiation from thunderstorms and lightning. The payload consisted of a suite of instruments designed to detect optical signals, electric fields, and gamma rays from lightning. Starting from Georgia, USA, 16 flights were performed, for a total of about 70 flight hours at a cruise altitude of 20 km. Of these, 45 flight hours were over thunderstorm regions. An analysis of two gamma ray glow events that were observed over Colorado at 21:47 UT on 8 May 2017 is presented. We explore the charge structure of the cloud system, as well as possible mechanisms that can produce the gamma ray glows. The thundercloud system we passed during the gamma ray glow observation had strong convection in the core of the cloud system. Electric field measurements combined with radar and radio measurements suggest an inverted charge structure, with an upper negative charge layer and a lower positive charge layer. Based on modeling results, we were not able to unambiguously determine the production mechanism. Possible mechanisms are either an enhancement of cosmic background locally (above or below 20 km) by an electric field below the local threshold or an enhancement of the cosmic background inside the cloud but then with normal polarity and an electric field well above the Relativistic Runaway Electron Avalanche threshold.

The intracellular target for the antiresorptive aminobisphosphonate drugs in Dictyostelium discoideum is the enzyme farnesyl diphosphate synthase.

Aminobisphosphonate (aBP) drugs inhibit osteoclast-mediated bone resorption and also growth of amoebas of Dictyostelium discoideum apparently by interaction with the same intracellular target. Identification of the target in Dictyostelium therefore could also identify the target in osteoclasts. The aBPs (100 microM alendronate and 30 microM YM-175) inhibited conversion of [14C]mevalonate into sterols by cultures of Dictyostelium amoebas. One of three enzymes (isopentenyl diphosphate [IDP] isomerase, farnesyl diphosphate [FDP] synthase, and squalene synthase) appeared to be the target for this inhibition because conversion of [14C]IDP into squalene, the immediate precursor for sterol biosynthesis, was inhibited in extracts of wild-type amoebas by alendronate (IC50 = 75 nM) or risedronate (IC50 = 30 nM) whereas, when the extract had been prepared from amoebas of strains selected for having partial resistance to the growth-inhibitory effects of alendronate (strain MR102) or risedronate (strain RB101), the values of IC50 were increased to 700 nM for alendronate (MR102 extract) or 130 nM for risedronate (RB101 extract). Neither IDP isomerase nor squalene synthase was inhibited significantly by alendronate or risedronate but both of these aBP drugs, and all others tested, inhibited FDP synthase. Determination of the nucleotide sequences of complementary DNAs (cDNAs) encoding FDP synthase in the wild-type and aBP-resistant strains of Dictyostelium indicated that there had been no changes in the amino acid sequence of the enzyme in the mutant strains. However, both mutant strains overproduce FDP synthase. It is concluded that FDP synthase is the intracellular target for the aBP drugs.

Fermi LARGE AREA TELESCOPE OBSERVATIONS OF BLAZAR 3C 279 OCCULTATIONS BY THE SUN.

Observations of occultations of bright γ-ray sources by the Sun may reveal predicted pair halos around blazars and/or new physics, such as, e.g., hypothetical light dark matter particles-axions. We use Fermi Gamma-Ray Space Telescope (Fermi) data to analyze four occultations of blazar 3C 279 by the Sun on October 8 each year from 2008 to 2011. A combined analysis of the observations of these occultations allows a point-like source at the position of 3C 279 to be detected with significance of ≈3σ, but does not reveal any significant excess over the flux expected from the quiescent Sun. The likelihood ratio test rules out complete transparency of the Sun to the blazar γ-ray emission at a 3σ confidence level.