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Solar Energetic Proton Fluxes in Near-Earth Space on March 13-23, 2023
DOI: 10.1134/S0010952523600282 Bibcode: 2024CosRe..62..197V

Vlasova, N. A.; Bazilevskaya, G. A.; Ginzburg, E. A. +5 more

The results of studying the fluxes of solar protons with energies greater than 5 MeV in near-Earth space on March 13-23, 2023, are presented. The features of the period under study are no visible solar flare with which the beginning of the event could be associated and an untypical time profile of proton fluxes, as well as a long duration of the e…

2024 Cosmic Research
SOHO SolarOrbiter 2
Earth's Ionospheric Response to Solar Activity Phenomena in February-March 2023
DOI: 10.1134/S0010952523600294 Bibcode: 2024CosRe..62..187V

Sheiner, O. A.; Vybornov, F. I.

As a result of the analysis of data from vertical and oblique sounding of the ionosphere in February-March 2023 using the new ionospheric index, it was found that solar coronal mass ejections (CMEs) of the loop type lead to a long-term decrease in the critical frequencies F-layer of the ionosphere, while other types of CMEs may not lead to signifi…

2024 Cosmic Research
SOHO 0
New 1.38-µm Water Vapor Band Spectroscopy for a CO2 Atmosphere: H2O Measurements in the Martian Atmosphere in the SPICAM/MEX and ACS NIR/TGO Experiments
DOI: 10.1134/S0010952524601282 Bibcode: 2024CosRe..62S...1F

Montmessin, F.; Fedorova, A. A.; Korablev, O. I. +5 more

The H2O 1.38-µm band has been used to measure water vapor in the Martian atmosphere since the MAWD (Mars Atmospheric Water Detector) experiment on Viking-1 and -2. Currently, two experiments in orbit around Mars—SPICAM IR (SPectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars InfraRed) on Mars Express and A…

2024 Cosmic Research
MEx 0
Geomagnetic Pulsations in the 1-4 mHz Frequency Range (Pc5/Pi3) in the Magnetotail. Internal and Extramagnetospheric Sources
DOI: 10.1134/S0010952524600355 Bibcode: 2024CosRe..62..323Y

Yagova, N. V.; Evsina, N. S.

Spectral and spatial parameters of nonstorm Pc5/Pi3 geomagnetic pulsations in the geomagnetic tail are studied based on magnetic measurements on Cluster satellites under different conditions in the interplanetary medium. Both the average values of the magnetic field components in front of the bow shock and fluctuations in the pulsations' frequency…

2024 Cosmic Research
Cluster 0
Coronal Propagation of Solar Protons during and after Their Stochastic Acceleration
DOI: 10.1134/S0010952523700235 Bibcode: 2023CosRe..61..232G

Logachev, Yu. I.; Struminsky, A. B.; Grigorieva, I. Yu. +1 more

Solar protons in eruptive flares are stochastically accelerated in a wide spatial angle, and then they are effectively kept behind the expanding coronal mass ejection (CME) front, which can either bring protons to the magnetic-field line going to a remote observer or carry them away. We consider 13 solar proton events of cycle 24 in which protons …

2023 Cosmic Research
INTEGRAL 5
High-Cadence Observations of Magnetic Field Dynamics and Photospheric Emission Sources in the Eruptive Near-the-Limb X4.9 Solar Flare on 25 February, 2014: Evidences for Two-Stage Magnetic Reconnection during the Impulsive Phase
DOI: 10.1134/S0010952523090010 Bibcode: 2023CosRe..61..265S

Zimovets, I. V.; Sharykin, I. N.; Radivon, A. V.

We present an analysis of the pre-limb eruptive X4.9 solar flare on February 25, 2014, by means of which we confirm a hypothesis of the two-stage energy release corresponding to two magnetic reconnection regimes in the flare impulsive phase. This flare is selected, firstly, because of its morphological peculiarities suggesting the presence of the …

2023 Cosmic Research
PROBA-2 1
The Influence of Oxygen Ions on the Formation of a Thin Current Sheet in the Magnetotail
DOI: 10.1134/S0010952523700259 Bibcode: 2023CosRe..61..218D

Malova, H. V.; Popov, V. Yu.; Zelenyi, L. M. +2 more

A thin current sheet in the Earth's magnetotail with characteristic thickness of one to several proton gyroradii is often observed during magnetospheric disturbances named substorms, when a relatively thick current configuration in the magnetotail is narrowed to an extremely small thickness and then can spontaneously be destroyed. The current-shee…

2023 Cosmic Research
Cluster 0
Estimation of the Electron Density in the Near 3-4 RE Magnetosphere Based on the Measurement of the Interball-2 Satellite Potential
DOI: 10.1134/S0010952523700193 Bibcode: 2023CosRe..61..206S

Smirnova, N. F.; Stanev, G.

A new method is proposed for determining the electron density in rarefied plasma, based on simultaneous measurements of the Interball-2 satellite potential using IESP-2 (electric field instrument) and KM-7 (electron temperature sensor) probe devices. This makes it possible to estimate the photoelectron current density based on a procedure proposed…

2023 Cosmic Research
Cluster 0
Catalogs of Solar Proton Events as a Tool for Studying Space Weather
DOI: 10.1134/S001095252203008X Bibcode: 2022CosRe..60..151V

Vlasova, N. A.; Bazilevskaya, G. A.; Ginzburg, E. A. +8 more

Distinguishing features of a series of solar proton event (SPE) catalogs for the 20th-24th cycles of solar activity are described. The results of a comparative analysis of the 23rd and 24th cycles of solar activity performed according to the data of a series of SPE catalogs are presented. The opportunities provided by SPE catalogs for studying spa…

2022 Cosmic Research
SOHO 2
Physical Calibrations of the FREND Instrument Installed Onboard TGO Martian Orbiter
DOI: 10.1134/S0010952522010099 Bibcode: 2022CosRe..60...23M

Mitrofanov, I. G.; Golovin, D. V.; Litvak, M. L. +10 more

The article presents results of ground calibrations of the FREND neutron telescope installed onboard the TGO spacecraft of the Russian-European ExoMars project. The main goal of the FREND space experiment is to measure hydrogen content in the subsurface layer of Mars to a depth of 1 m. High resolution maps of water mass fraction in the regolith ar…

2022 Cosmic Research
ExoMars-16 1