The EUV Level 1 (L1) product containing EUV limb radiances has been updated to V3. This resolves primarily remaining issues with flatfielding. The Level 2 (L2) products are now re-run using these L1 inputs. The retrieval algorithm hasn't changed but the revision number has been indexed on the L2 products. This now extends the L2 products into 2021.

By Robert Sanders, UC Berkeley Media relations | June 1, 2018

If scientists hope to predict the magnetic storms around Earth that endanger satellites and interfere with radio communications on the ground, they must understand how tropical storms on Earth affect these magnetic storms 60 miles above our heads.

A new mission, NASA’s Ionospheric Connection Explorer (ICON), is charged with that very task: to measure the winds of ionized atoms at the edge of space and determine how they are impacted by atmospheric weather, in particular seasonal monsoons in the tropics.

The ICON mission is proceeding apace. High fives are in order since the team just completed its fourth operational readiness test (ORT). During an ORT, a dozen SSL Mission Operation Team Members join forces with two dozen spacecraft engineers from Orbital ATK to rehearse the first week of activities that will occur during ICON’s launch and early orbit. It’s an entire week of long days and intensive testing in ICON’s Mission Operations Center at the UC Berkeley Space Sciences Lab, to simulate operation of the observatory. Spurred along by the fact that this was the final ORT before launch, the team worked together to bring it to a healthy and successful completion (simulating operations with a failed momentum wheel, no less). The next time these teams come together at SSL will be the actual launch day for ICON.

Dr. Manfred Bester, Manager of Mission Operations Center at the Space Sciences Lab of UC Berkeley, explains what he and his team do to prepare for the upcoming ICON launch.

"The most intense part is the immediate time before launch."