Magnetospheric Venus Space Explorers (MVSE) mission: A proposal for understanding the dynamics of induced magnetospheres

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Magnetospheric Venus Space Explorers (MVSE) mission: A proposal for understanding the dynamics of induced magnetospheres

Alpbach Summer School 2022

European Space Agency Concurrent Engineering Academy 2022

Induced magnetospheres form around planetary bodies with atmospheres through the interaction of the solar wind with their ionosphere. Induced magnetospheres are highly dependent on the solar wind conditions and have only been studied with single spacecraft missions in the past. Without simultaneous measurements of solar wind variations and phenomena in the magnetosphere, establishing a link between both can only be done indirectly, using statistics over a large set of measurements. This gap in knowledge could be addressed by a multi-spacecraft plasma mission, optimized for studying global spatial and temporal variations in the magnetospheric system around Venus, which hosts the most prominent example of an induced magnetosphere in our solar system. The MVSE mission comprises four satellites, of which three are identical scientific spacecraft, carrying the same suite of instruments probing different regions of the induced magnetosphere and the solar wind simultaneously. The fourth spacecraft is the transfer vehicle which acts as a relay satellite for communications at Venus. In this way, changes in the solar wind conditions and extreme solar events can be observed, and their effects can be quantified as they propagate through the Venusian induced magnetosphere. Additionally, energy transfer in the Venusian induced magnetosphere can be investigated. The scientific payload includes instrumentation to measure the magnetic field, electric field, and ion–electron velocity distributions. This study presents the scientific motivation for the mission as well as requirements and the resulting mission design. Concretely, a mission timeline along with a complete spacecraft design, including mass, power, communication, propulsion and thermal budgets are given. This mission was initially conceived at the Alpbach Summer School 2022 and refined during a week-long study at ESA’s Concurrent Design Facility in Redu, Belgium.”


About Crisel Suarez
Crisel Suarez

Hi I am Crisel Suarez!

Email : criselsuarez[at]gmail[dot]com

Website : https://criselsuarez.github.io/

About Crisel Suarez

¡Hola! My name is Crisel Suarez. I am a Physics PhD candidate at Vanderbilt University and Smithsonian Astrophysical Observatory Predoctoral Fellow . I grew up in Mexico City, Mexico and Austin, TX, USA. I am fully bilingual in both Spanish and English. I earned my Bachelor’s of Science and majored in Mathematics and minored in Global Studies and Physics at a small liberal arts school called St. Edward’s University . I was a McNair Scholar at St. Edward’s University and pursued all types of research; from Computer Science looking at the expected values of properties in the game of Monopoly (with Dr. Michael Kart ), Mathematics looking at the tetrominoes ( TETRIS pieces) and how they form gaps and make you lose at TETRIS (with Dr. Jason Callahan ), and Science Education in quantifying science literacy in undergraduates students (with Dr. Paul Walter . I also took a graduate Nanotechnologies and Nanofabrication certification from the Nanomanufacturing Systems Center (NASCENT) at University of Texas at Austin.

After graduating from St. Edward’s University, I went to pursue my Masters of Science in Physics at Fisk University as part of the Fisk-Vanderbilt Masters to PhD program . At Fisk, I was part of Dr. Arnold Burger’s Materials Science and Applications Group (MSAG) where I studied the chemical composition of high energy crystal scintillators using Vanderbilt’s University high performance computing ACCRE facilities.

During the summers as a Masters student, I had the opportunity to work with Dr. Christopher S. Moore at the Center for Astrophysics | Harvard & Smithsonian in the Solar Stellar X-ray Group as part of the Fisk-Vanderbilt-CfA Latino Initiative Program (now CfA Research Experiences in Astronomy, Technology, & Engineering (CREATE) program. I worked on analyzing beautiful high energy events in the Sun called solar flares . As part of PhD work at Vanderbilt University, I continued to examined ~30 soft x-ray (SXR) flares observed with the Miniature X-ray Solar Spectrometer (MinXSS-1) and derived changes in temperature, volume emission measure and elemental abundances as a function of time with parametric spectral fits. I continue to research solar flares and look for Quasi-Periodic Pulsations (QPPs) in flares with different instruments including Hinode/X-ray Telescope (Hinode/XRT) , Solar Dynamic Observatory/Atmospheric Imaging Assembly (SDO/AIA) , Geostationary Operational Environmental Satellite (GOES) , Miniature X-ray Solar Spectrometer- 1 and 2 (MinXSS-1&2) and Dual Aperture X-ray Solar Spectrometer (DAXSS). I have also used the Hydrodynamic Radiation (HYDRAD) model to synthesize Extreme Ultraviolet (EUV) and soft x-ray (SXR) emission in solar flares.

I also enjoy engaging in science outreach events, promoting research, curiosity, creativity and mentoring the next generation of scientists!

When I have some rare free time, I like going to museums, shows, trying new foods, and traveling!

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