Radio Wave Propagation (IZMIRAN)
Identifiers
- name variant Radio Wave Propagation (IZMIRAN) 0.60 · backfill
Papers (12)
- Long- and Mid-Term Variations of the Soft X-ray Flare Type in Solar Cycles astro-ph.SR · 2017 · author #4
- An Early Diagnostics of the Geoeffectiveness of Solar Eruptions from Photospheric Magnetic Flux Observations: The Transition from SOHO to SDO astro-ph.SR · 2017 · author #6
- Relations between Microwave Bursts and near-Earth High-Energy Proton Enhancements and their Origin astro-ph.SR · 2015 · author #9
- A Simple Way to Estimate the Soft X-ray Class of Far-Side Solar Flares Observed with STEREO/EUVI astro-ph.SR · 2015 · author #5
- Responsibility of a Filament Eruption for the Initiation of a Flare, CME, and Blast Wave, and its Possible Transformation into a Bow Shock astro-ph.SR · 2014 · author #15
- Relationship between the Magnetic Flux of Solar Eruptions and the Ap Index of Geomagnetic Storms astro-ph.SR · 2014 · author #7
- A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. IV. Unusual Magnetic Cloud and Overall Scenario astro-ph.SR · 2014 · author #12
- A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. III. Catastrophe of the Eruptive Filament at a Magnetic Null Point and Formation of an Opposite-Handedness CME astro-ph.SR · 2014 · author #12
- A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. II. CMEs, Shock Waves, and Drifting Radio Bursts astro-ph.SR · 2013 · author #15
- Relations between strong high-frequency microwave bursts and proton events astro-ph.SR · 2013 · author #9
- Microwave Negative Bursts as Indications of Reconnection between Eruptive Filaments and Large-Scale Coronal Magnetic Environment astro-ph.SR · 2013 · author #11
- Heating the Solar Atmosphere by the Self-Enhanced Thermal Waves Caused by the Dynamo Processes physics.plasm-ph · 2012 · author #3
Mentions
- 1511.05839 #9 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1505.01649 #5 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1410.8696 #15 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1410.1646 #7 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1409.0283 #12 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1404.3515 #12 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1308.3010 #15 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1308.2275 #9 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1307.6965 #11 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
- 1201.4990 #3 · backfill · confidence 0.70 Radio Wave Propagation (IZMIRAN)
Frequent Coauthors
- Ionosphere 12 shared papers
- Irkutsk 10 shared papers
- Moscow 10 shared papers
- Russia 9 shared papers
- Russia) 9 shared papers
- Troitsk 9 shared papers
- (2) Pushkov Institute of Terrestrial Magnetism 5 shared papers
- (2) Institute of Solar-Terrestrial Physics SB RAS 3 shared papers
- (3) P.N. Lebedev Physical Institute 3 shared papers
- I.M. Chertok (1) 3 shared papers
- V.V. Grechnev (1) 3 shared papers
- A. M. Uralov (1) 2 shared papers
- A.M. Uralov (1) 2 shared papers
- B.P. Filippov (2) 2 shared papers
- I.M. Chertok (2) 2 shared papers
- V. Grechnev (1) 2 shared papers
- V. V. Grechnev (1) 2 shared papers
- ((1) Pushkov Institute of Terrestrial Magnetism 1 shared papers
- (2) Ussuriysk Astrophysical Observatory 1 shared papers
- (3) Pushkov Institute of Terrestrial Magnetism 1 shared papers