Работы, цитирующие эту работу

Работ: 3

Работа: How is open solar magnetic flux lost over the solar cycle?

1. Mass loss via solar wind and coronal mass ejections during solar cycles 23 and 24

   Wageesh Mishra, Nandita Srivastava, Yuming Wang +3

   СтатьяSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society2019Цитирований: 1

   ABIABI:AkademIndex/openalex/2019.article.000098

2. Dynamo in the Outer Heliosheath: Necessary Conditions

   E. S. Belenkaya

   СтатьяSolar and Space Plasma DynamicsSolar Physics2015Цитирований: 0

   ABIABI:AkademIndex/openalex/2015.article.000271

3. Solar Wind Mass‐Loss Rate and Its Dependence on Open Solar Magnetic Flux During Solar Cycles 23–25

   Zavkiddin Mirtoshev, Akmal Safarov, Shakhboz Khasanov

   СтатьяSolar and Space Plasma DynamicsAstronomische Nachrichten2026Цитирований: 0

   ABIABI:AkademIndex/openalex/2026.article.012451