[Robert Sanders, Berkeley News, October 10, 2019] At 9:59 p.m. EDT this evening, Thursday, Oct. 10, NASA launched the Ionospheric Connection, or ICON, mission, putting into orbit a satellite built largely at UC Berkeley’s Space Sciences Laboratory to explore the dynamic region where Earth meets space, the ionosphere.

The mission is the first dedicated to studying how terrestrial weather can help drive space weather above, in the region where our upper atmosphere overlaps with the lowest reaches of space – a dynamic region where changes can disrupt radio, cell phone, and GPS communications used to guide airplanes and ships.

While all went smoothly at the launch site over the Atlantic, mission control at the Space Sciences Laboratory had to contend with a power outage instituted by the local utility, Pacific Gas & Electric, to prevent predicted high winds from sparking fires in the surrounding Berkeley hills. The campus’s cogeneration plant supplied the needed power to track the satellite during its initial passes over California.

“It was like watching a choreographed performance turn into a jazz improvisation as problems come up and the individual team members solved them in real time feeding off one another’s talent and energy,” said astronomer Steve Beckwith, director of the lab.

[NASA press release] After successfully launching Thursday night, NASA’s Ionospheric Connection Explorer (ICON) spacecraft is in orbit for a first-of-its-kind mission to study a region of space where changes can disrupt communications and satellite orbits, and even increase radiation risks to astronauts.

A Northrop Grumman Stargazer L-1011 aircraft took off at 8:31 p.m. EDT from Cape Canaveral Air Force Station in Florida carrying ICON, on a Northrop Grumman Pegasus XL rocket, to launch altitude of about 39,000 feet. The first launch opportunity around 9:30 was skipped due to communication issues between the ground team at Cape Canaveral and the aircraft. On the second attempt, the aircraft crew released its payload at 9:59 p.m. EDT and automated systems on the Pegasus rocket launched ICON, a spacecraft roughly the size of a refrigerator, into space.

The spacecraft’s solar panels successfully deployed, indicating it has power with all systems operating. After an approximately month-long commissioning period, ICON will begin sending back its first science data in November.

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.

Designed and built at the Space Sciences Laboratory of UC Berkeley, ICON is scheduled for a June 14 launch from an airplane over the Pacific Ocean, and should start probing the upper atmosphere and ionosphere by August.

“We are built to catch everything that is coming up into space at the boundary of space,” said Thomas Immel, principle investigator for the mission and a physicist at the Space Sciences Laboratory. “Anything that comes past there we are going to see.”

- Robert Sanders, Berkeley News.  Scientists at UC Berkeley’s Space Sciences Laboratory are preparing for the 2017 launch of an Earth-orbiting satellite to discover how storms in the atmosphere affect storms in the ionosphere.

The ionosphere is the edge of space where the sun ionizes the air in Earth’s atmosphere to create constantly shifting streams and sheets of charged particles.

The NASA-funded satellite, called the Ionospheric Connection Explorer, or ICON, will complement observations from a sister satellite also scheduled for launch in 2017: the Global Observations of the Limb and Disk, or GOLD. GOLD is being led by the University of Central Florida, though UC Berkeley space scientist Scott England works on both missions.

-- December 16, 2015

The warm El Niño conditions affecting weather around the Pacific Ocean are also affecting conditions in space, according to University of California, Berkeley scientists.

El Niño is commonly observed as a global change in rainfall due to changes in temperature in the Pacific Ocean. However, UC Berkeley scientists report today at the annual meeting of the American Geophysical Union meeting in San Francisco that the processes that lead to increased precipitation are also driving unexpected changes in the ionosphere, the uppermost level of the atmosphere.

The findings (AGU abstract #SA31F-2383) will be presented by Dr. Thomas Immel, and are based on calculations by Dr. Astrid Maute of the High Altitude Observatory in Boulder, Colorado.

“We expected that we would see some changes in the ionosphere when we started this study” says Dr. Immel, a Senior Fellow at UC Berkeley’s Space Sciences Laboratory, “but we were shocked at how strong the effect has turned out to be”.