Electron energy measurements in pulsating auroras

1981 ◽  
Vol 59 (8) ◽  
pp. 1106-1115 ◽  
Author(s):  
D. J. McEwen ◽  
E. Yee ◽  
B. A. Whalen ◽  
A. W. Yau

Electron spectra were obtained during two rocket flights into pulsating aurora from Southend, Saskatchewan. The first rocket launched at 1143:24 UT, on February 15, 1980 flew into an aurora of background intensity 275 R of N2+ 4278 Å and showing regular pulsations with about a 17 s period. Electron spectra of Maxwellian energy distributions were observed with an average E0 = 1.5 keV, rising to 1.8 keV during the pulsations. There was one-to-one correspondence between the electron energy modulation and the observed optical pulsations. The second rocket, launched at 1009:10 UT on February 23, flew into a diffuse auroral surface of intensity 800 R of N2+ 4278 Å and with somewhat irregular pulsations. The electron spectra were again of Maxwellian energy distribution with an average E0 = 1.8 keV increasing to 2.1 keV during the pulsations. The results from these flights suggest that pulsating auroras occurring in the morning sector may be quite commonly excited by low energy electrons. The optical pulsations are due to periodic increases in the energy of the electrons with the source of modulation in the vicinity of the geomagnetic equatorial plane.

2020 ◽  
Vol 496 (4) ◽  
pp. 5518-5527
Author(s):  
N Sahakyan

ABSTRACT The origin of the multiwavelength emission from the high-synchrotron-peaked BL Lac 1ES 1218+304 is studied using the data from SwiftUVOT/XRT, NuSTAR, and Fermi-LAT. A detailed temporal and spectral analysis of the data observed during 2008–2020 in the  γ-ray (>100 MeV), X-ray (0.3–70 keV), and optical/UV bands is performed. The γ-ray spectrum is hard with a photon index of 1.71 ± 0.02 above 100 MeV. The SwiftUVOT/XRT data show a flux increase in the UV/optical and X-ray bands; the highest 0.3–3 keV X-ray flux was (1.13 ± 0.02) × 10−10 erg cm−2 s−1. In the 0.3–10 keV range, the averaged X-ray photon index is >2.0 which softens to 2.56 ± 0.028 in the 3–50 keV band. However, in some periods, the X-ray photon index became extremely hard (<1.8), indicating that the peak of the synchrotron component was above 1 keV, and so 1ES 1218+304 behaved like an extreme synchrotron BL Lac. The hardest X-ray photon index of 1ES 1218+304 was 1.60 ± 0.05 on MJD 58489. The time-averaged multiwavelength spectral energy distribution is modelled within a one-zone synchrotron self-Compton leptonic model using a broken power law and power law with an exponential cutoff electron energy distributions. The data are well explained when the electron energy distribution is $E_{\rm e}^{-2.1}$ extending up to γbr/cut ≃ (1.7 − 4.3) × 105, and the magnetic field is weak (B ∼ 1.5 × 10−2 G). By solving the kinetic equation for electron evolution in the emitting region, the obtained electron energy distributions are discussed considering particle injection, cooling, and escape.


1990 ◽  
Vol 68 (2) ◽  
pp. 166-169 ◽  
Author(s):  
Mohammad F. Mahmood

An investigation was made of the process of dissociative excitation of a HgCl radical in the B2Σ+1/2 state due to collisions of low-energy electrons with HgCl2 and CH3HgCl molecules. Using the most intense band of the B2Σ+1/2 – X2Σ+1/2 system of the HgCl radical at 557 nm that corresponds to the ν′ = 0 to ν″ = 22 transition, emission cross sections were measured in the electron energy range 1–100 eV. The threshold electron energy for the observation of the B2Σ+1/2 – X2Σ+1/2 band system has been determined to be 7.0 and 8.0 eV for HgCl2 and CH3HgCl molecules, respectively.


2006 ◽  
Vol 527-529 ◽  
pp. 481-484 ◽  
Author(s):  
W. Sullivan ◽  
John W. Steeds

Samples of 4H SiC, both n- and p-doped, have been irradiated with low-energy electrons in a transmission electron microscope. The dependence of the silicon vacancy-related V1 ZPL doublet (~860nm) on electron energy and electron dose has been investigated by low temperature photoluminescence spectroscopy. Furthermore, this luminescence centre has been studied across a broad range of samples of various doping levels. Some annealing characteristics of this centre are reported.


A small probe which extracts a sample pencil from the distribution of ions and electrons in a low pressure arc has been used to carry out a retardation energy distribution analysis on these particles. Axial and radial variations in these distributions in a striated hydrogen discharge have been studied. The results confirm the findings of Boyd & Twiddy for electrons and supplement their data with new information on the energy distributions of the positive ions. The measurements at the striation tail-head transition are in accord with Langmuir’s double sheath criterion.


The Druyvesteyn method of measuring electron energy distributions in low-pressure plasmas has been applied to the cathode region of hot cathode discharges in helium, neon and argon at a pressure of 0·05 mm Hg. In all gases the column was striated. In helium and neon, measurements in the striation nearest the cathode show two well separated groups of electrons, the more energetic or primary electrons arising from the Langmuir double space-charge sheath at the filament; the lower-energy group or secondary electrons being produced by the primary electrons in inelastic collisions. The concentrations of both groups fall off with increasing distance from the filament, but their separation and energy spread is constant throughout the striation indicating the absence of any energy exchanging process capable of appreciably modifying the energy distribution. It would appear therefore that the energy-exchanging processes observed by Langmuir (1925), by Merrill & Webb (1939), and by Gabor, Ash & Dracott (1955) were inoperative in the discharges employed in the present experiments. In the absence of an energy-exchanging process a uniform column cannot arise at the pressures employed, since in order to give rise to a truly uniform column the axial field must extend over many mean free paths, a condition which is not fulfilled in these discharges, since the entire discharge tube is less than 100 mean free paths long and thus on the average an electron makes fewer than 1000 collisions between cathode and anode. The application of an axial field simply augments the energy of the electrons without modifying the broad features of the energy distribution. If therefore the energy distribution consists of two separate groups of electrons a uniform field can maintain the discharge while primary electrons remain, but when these are exhausted, because of the distinct separation between the primary and secondary groups, new primary electrons can only be created by a step of potential. Under these conditions the striated column will exist and a transition to a stable uniform column is only to be expected when a mechanism exists for modifying the energy distribution in a few mean free paths. Measurements at higher currents in helium and neon show a definite tendency for the trough between the two groups to be eliminated; this is presumably due to secondary processes. The presence of a high metastable concentration enables both primary and secondary groups to be modified by secondary collisions thus eliminating the sharp demarcation between the two groups which was evident at lower currents. It seems possible also that the disposition of the first critical potential in a gas may influence its ability to develop a uniform column, since if the first excitation potential is appreciably less than half the ionization potential the primary and secondary groups will overlap. This might be effective in the metal vapours. The probable influence of impurities on the appearance of the discharge and the energy distribution are considered on the basis of the data available from measurements in hydrogen, helium and neon. Measurements in the negative regions in argon, while showing features characteristic of the striated column, were quite different in character from the other rare gases in that a fairly strong but decreasing field existed in the tube. Measurements here show very clearly how a uniform field augments the energy of the electrons without modifying the broad features of the distribution.


2019 ◽  
Vol 20 (14) ◽  
pp. 3496 ◽  
Author(s):  
Rebecca Meißner ◽  
Linda Feketeová ◽  
Eugen Illenberger ◽  
Stephan Denifl

Misonidazole (MISO) was considered as radiosensitizer for the treatment of hypoxic tumors. A prerequisite for entering a hypoxic cell is reduction of the drug, which may occur in the early physical-chemical stage of radiation damage. Here we study electron attachment to MISO and find that it very effectively captures low energy electrons to form the non-decomposed molecular anion. This associative attachment (AA) process is exclusively operative within a very narrow resonance right at threshold (zero electron energy). In addition, a variety of negatively charged fragments are observed in the electron energy range 0–10 eV arising from dissociative electron attachment (DEA) processes. The observed DEA reactions include single bond cleavages (formation of NO2−), multiple bond cleavages (excision of CN−) as well as complex reactions associated with rearrangement in the transitory anion and formation of new molecules (loss of a neutral H2O unit). While any of these AA and DEA processes represent a reduction of the MISO molecule, the radicals formed in the course of the DEA reactions may play an important role in the action of MISO as radiosensitizer inside the hypoxic cell. The present results may thus reveal details of the molecular description of the action of MISO in hypoxic cells.


1994 ◽  
Vol 159 ◽  
pp. 358-359
Author(s):  
Luis Salas ◽  
Irene Cruz-González ◽  
Luis Carrasco

We develop a new method called “Inverse Synchrotron Transform” (IST) to study the spectral energy distributions of AGNs. We demonstrate that it is possible to use Bayes Theorem for conditional probabilities to derive a self-consistent solution for the electron energy distribution (EEDs), starting from the observed spectral energy distributions (SEDs) and the assumption that the only physical process involved is thin synchrotron radiation. We test the IST method and find that it allows to distinguish among different EEDs that produce SEDs which nevertheless seem very similar. We apply the method to multifrequency simultaneous observations of AGNs (paper II, this conference).


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