Global Structure of the Solar Wind in a of Decreasing Solar Activity from Interplanetary-Scintillation Monitoring Data
- Authors: Chashei I.V.1, Tyul’bashev S.A.1, Subaev I.A.1, Izvekova V.A.1
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Affiliations:
- Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
- Issue: Vol 63, No 2 (2019)
- Pages: 161-165
- Section: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/193137
- DOI: https://doi.org/10.1134/S1063772919020021
- ID: 193137
Cite item
Abstract
An analysis of data from three years of monitoring of interplanetary scintillations in 2015–2017 during a phase of decreasing solar activity is presented. The observations were carried out on the Large Scanning Antenna of the Lebedev Physical Institute at 111 MHz. During the period considered, the spatial distriution of the scintillation level was close to spherically symmetrical, on average, and did not undergo any strong time variations on scales of months or years. The monthly-mean scintillation level is not correlated with theWolf number.
About the authors
I. V. Chashei
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Author for correspondence.
Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
S. A. Tyul’bashev
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
I. A. Subaev
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
V. A. Izvekova
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute
Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast, 142290
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