Roscosmos Ionosfera science mission to launch atop Soyuz from Vostochny  Cosmodrome
Date:
Thu, 24 Jul 2025 21:04:03 +0000
Description:
A Soyuz 2.1b rocket is set to launch from Site 1S at Vostochny Cosmodrome in  The post Roscosmos Ionosfera science mission to launch atop Soyuz from  Vostochny Cosmodrome appeared first on NASASpaceFlight.com .
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A Soyuz 2.1b rocket is set to launch from Site 1S at Vostochny Cosmodrome in  Russia, carrying two Ionosfera-M satellites into a Sun-synchronous orbit.  Launch is scheduled for Friday, July 25, at 05:54 UTC and will see Soyuz fly  on a northern trajectory over vast but sparsely populated territory. 
The Ionosfera-M no. 3 and no. 4 satellites are to fly to a circular orbit  around 800 km altitude on a Fregat-M upper stage to complete the  four-satellite Ionosfera science satellite constellation. The Ionosfera-M no.  1 and no. 2 satellites were launched in November 2024 aboard a similar  Soyuz/Fregat launch vehicle from Vostochny. 
 
The Soyuz rocket will also carry 18 secondary payloads on this flight, with 
17 of them being Russian and one from the Iranian Space Agency. One of the  Russian satellites is a 16U CubeSat, while 16 3U CubeSats are flying for 
three different Russian commercial organizations. Irans Nahid-2  telecommunications satellite will also be launched. The Soyuz 2.1b/Fregat-M  vehicle for the Ionosfera 3/4 mission during processing. (Credit: TSENKI) 
This flight will be only the third Soyuz 2.1b flight of 2025 and the first  launch of the year from Vostochny. Russia developed the Vostochny Cosmodrome  as a domestic alternative to the Baikonur Cosmodrome in Kazakhstan. Russia is  leasing the cosmodrome from the Kazakh government, paying $115 million USD 
per year to lease Baikonur until 2050. See Also Ionosfera-M 3&4 Updates  Russian Spaceflight Section NSF Store Click here to Join L2 
Roscosmos initiated the Ionosfera-M constellation as part of Project 
Ionozond, a program designed to study the geophysical environment around 
Earth as well as space weather and its effects on our planet. Four Ionosfera  satellites were developed and procured for these studies, while a fifth  satellite was also proposed. 
The fifth satellite for this project, known as Zond-M, is designed to observe  the Sun from a Sun-synchronous orbit (SSO) around Earth. However, the Zond-M  portion of the project was suspended in late 2024 due to budget cuts.  Roscosmos has faced funding shortfalls in recent years due to the Russian  invasion of Ukraine and its demands on the countrys resources. 
The overall Ionozond project is managed by Roscosmos in cooperation with the  All-Russian Scientific Research Institute of Electromechanics (JSC VNIIEM),  the Russian Federal Service for Hydrometeorology and Environmental Monitoring  (Roshydromet), and the Russian Academy of Sciences. Roshydromet will use data  from Ionosfera-M for space weather forecasting, while JSC VNIIEM developed 
and built the satellites. 
The Ionosfera satellites, each massing roughly 400 kg, are designed for an  eight-year service life. The first pair of Ionosfera satellites was launched  into SSO with an ascending node corresponding to roughly 21:00 hours on the  evening terminator of Earth, while the second pair will be launched into an  orbital plane 90 degrees away from the first pair. The Ionosfera-M 3 and 4  satellites during processing. (Credit: TSENKI) 
The second pair will orbit along a line corresponding to the afternoon hours   roughly 15:00 hours  at the orbits ascending node. This will enable the  overall constellation to collect measurements of Earths ionosphere at  different times of the day. The measurements will be obtained by nine  instruments aboard each spacecraft. 
These instruments include four spectrometers, a short-wave sounder, a  magnetometer, an energetic particle sensor, and a radio-wave sounder. The  Ionospheric Plasma Energy Spectrometer (ESIP), the Plasma and Energetic  Radiation Spectrometer (SPER/1), the Galactic Cosmic Ray Spectrometer  (GALS/1), and the Gamma Spectrometer (SG/1) will study different aspects of  the ionospheres plasma, particles, and radiation. 
ESIP will measure the ionospheric plasma and study the ionospheres structure,  while SPER/1 will measure differential energy spectra of low-energy electrons  and protons. GALS/1 will measure proton flux energy as well as total proton  and electron fluxes, while SG/1 will study hard X-ray and gamma radiation in  Earths atmosphere. 
In addition to the four spectrometers, five other instruments will take  complementary measurements. The Ozonometer-TM short-wave sounder will measure  solar ultraviolet (UV) radiation reflected by Earths atmosphere, while the  low-frequency wave complex (NVK2) magnetometer will measure magnetic and  electric fields of near-Earth space. An Ionosfera satellite in processing.  (Credit: TSENKI) 
The GPS total electron content receiver (PES) will observe the altitude  distribution of electrons in Earths ionosphere, and the Laertes radio wave  sounder will measure electron density and total electron content. In 
addition, a dual-frequency beacon (MAYAK) will probe Earths ionosphere with  emphasis on the region not accessible by satellites. 
Though the Ionosfera satellites will not communicate with each other, they  will use an onboard science and data collection system to store and transmit  the science data obtained by the satellites to ground stations in Russia. The  ESIP, SPER/1, GALS/1, SG/1, Ozonometer-TM, NVK2, PES, Laertes, and MAYAK  instruments are present on all four spacecraft. 
Earths atmosphere is divided into several layers, with the troposphere being  the lowest atmospheric layer and extending from sea level up to roughly 10 km  altitude. The stratosphere extends from approximately 10 km to 50 km in  altitude and contains Earths protective ozone layer. Illustration of the  layers of the Earths atmosphere. (Credit: NASA) 
After the stratosphere comes the mesosphere, which extends to roughly 85 km 
in altitude, and from there, the thermosphere rises to altitudes of 500 to  1000 km. Most meteors burn up in the mesosphere as they impact Earths  atmosphere at high velocities. 
The thermosphere absorbs high-energy X-rays and UV radiation, and many  satellites, including the International Space Station, orbit within the  thermosphere. Finally, the exosphere is where Earths atmosphere fizzles into  space, reaching up to 190,000 km from Earths surface  half the distance to 
the Moon. 
The ionosphere, extending roughly from 80 km to 650 km in altitude, is a set  of layers in the mesosphere and thermosphere where high-energy solar 
radiation strips electrons from atoms and molecules. These atoms and 
molecules become electrically charged ions as a result, and the ionized 
layers of the atmosphere not only create aurorae during solar storms but also  affect radio and navigation signals. Soyuz 2.1b rolls out to Site 1S at  Vostochny. (Credit: Roscosmos) 
The Ionosfera-M constellation is the latest effort by space agencies to study  the ionosphere, which was discovered in 1902 when Guglielmo Marconi conducted  radio experiments. While the Soviet Union flew missions to study the  ionosphere as part of its Kosmos series of satellites, Ionosfera-M will mark  the first major Russian effort to study space weather in many years. 
( Lead image: A Soyuz 2.1b with a Fregat-M upper stage on the pad at 
Vostochny Cosmodrome ahead of the Ionosfera-M 3/4 launch. Credit: Roscosmos) 
 
The post Roscosmos Ionosfera science mission to launch atop Soyuz from  Vostochny Cosmodrome appeared first on NASASpaceFlight.com .
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Link to news story: 
https://www.nasaspaceflight.com/2025/07/ionosfera-34-launch/
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