SunRISE Beauty Pass
- Visualizations by:
- Adriana Manrique Gutierrez and
- Krystofer Kim
- Produced by:
- Joy Ng
- View full credits
A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events.
A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events.
A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events.
A coronal mass ejection (CME) erupts from the Sun and sends Type II radio bursts ahead of it. SunRISE measures the radio bursts and transmits the data to NASA’s Deep Space Network. Type II radio bursts are the earliest indicators of shocks from a solar eruption and can provide information on solar energetic particle (SEP) events.
Credits
Please give credit for this item to:
NASA's Goddard Space Flight Center Conceptual Image Lab
Animators
- Adriana Manrique Gutierrez (KBRwyle) [Lead]
- Krystofer Kim (KBRwyle) [Lead]
Scientists
- Joseph Lazio (JPL)
- Justin Kasper (University of Michigan)
Producer
- Joy Ng (KBRwyle) [Lead]
Technical support
- Aaron E. Lepsch (ADNET)