ESA mission controllers react to solar flare (Forwarded)

ESA News
http://www.esa.int

15 December 2006

ESA mission controllers react to solar flare

An energetic storm on the Sun has forced ESA mission controllers to react to
anomalies or take action to avoid damage to spacecraft. Several missions,
including Integral, Cluster and Envisat, felt the storm's effects,
highlighting the need for ESA's ongoing development of space weather
forecasting tools.

The joint ESA/NASA spacecraft SOHO (Solar & Heliospheric Observatory) imaged
a large solar flare on 13 December that led to an energetic solar radiation
storm.

The flare, detected by the LASCO (Large Angle and Spectrometric Coronagraph
Experiment) spectrometer on board SOHO, gave rise to a powerful coronal mass
ejection (CME), a stream of fast-moving atomic particles, directed towards
Earth. The flare also generated X-rays.

The ejection arrived at Earth 14 December between 13:00-19:00 CET
(12:00-18:00 UTC), where it gave rise to a strong geomagnetic storm; initial
edges of the ejection were detected as early as 04:00 CET (03:00 UTC) on 13
December.

The coronal mass ejection came during a week of intense solar activity that
is not yet over. An additional peak event occurred during the night of 14
December, and ground controllers on several ESA missions have reported
varying effects on their spacecraft.

Four-spacecraft Cluster II mission was one of the most affected

"We saw three anomalies on 13 December. Cluster 1 had a minor instrument
anomaly, while Cluster 2 and 4 had on-board systems affected," says Juergen
Volpp, Spacecraft Operations Manager for Cluster at ESA's Space Operations
Centre (ESOC) in Germany. "The Attitude and Orbit Control unit on Cluster 2
lost power and autonomously switched over to its redundant unit, while the
High-Power Amplifier on Cluster 4 switched itself off. This was a new
occurrence which we hadn't seen before," he said.

"When you have a burst, the flux of very fast charged particles increases
dramatically. This can cause discharges in electronic components -- the
so-called 'single-event upsets' -- on the spacecraft, as well as damage or
loss of data in solid-state memories," says Volpp.

Volpp says he can't be certain that the increased energetic particle flux
triggered the anomalies, but their occurrence is strongly correlated with
the timing of the peak burst on 13 December. He expects the mission to be
operating normally again in a few days.

Envisat & Integral affected

Envisat also experienced an unexpected anomaly correlated with the particle
flux's arrival at Earth.

"Operation of the Envisat Payload Module Computer was autonomously
suspended, causing all payload instruments to be switched off. It happened
around 19:00 CET, just before the particle peak on the 13th," said Frank
Diekmann, Spacecraft Operations Manager for Envisat. "We are still in a
period of very high solar activity," he added.

Controllers working on Integral had perhaps the best sense of the recent
solar activity -- two of the mission's four instruments include the JEM-X
and IBIS experiments, sensitive to X-rays and charged particles,
respectively. However, they also had to take the most proactive action to
avoid damage to the spacecraft's sensitive sensors.

"JEM-X automatically switched itself into safe mode twice, and we manually
switched IRIS off to avoid over-exposure," says Michael Schmidt, Spacecraft
Operations Manager for Integral.

ESA deep space missions avoid harm

The flurry of activity for controllers working on ESA missions orbiting in
the region of the Earth was a direct result of Thursday's coronal mass
ejection heading more or less directly towards our planet.

"The mass ejection headed from the Sun to Earth and our planetary missions,
on the other hand, weren't affected," explains Paolo Ferri, Head of the
Solar and Planetary Missions Division at ESOC.

Ferri says that CME events are highly directional, and that by chance all
three of ESA's deep space missions, Mars Express, Venus Express and Rosetta,
happen to be oriented on the side of the Sun opposite to the Earth right
now. "Our interplanetary spacecraft didn't see anything," he adds.

However, radio signals transmitted from the three deep space missions must
pass by the Sun to reach Earth, and so flight control teams could in fact
notice the increased solar activity as higher-than-normal interference in
the signals received on the ground.

Improved space weather forecasting tools now in development

The recent solar activity highlights the ongoing need for accurate space
weather forecasting and warning systems, so that spacecraft operators can
take action to protect instruments and systems hours or even minutes before
a peak of radiation or particles passes.

ESOC's Mission Control Technologies unit is working with the Institute for
the Development of New Technologies, an academic institute in Caparica,
Portugal, and Deimos Engenharia, a private company, in Lisbon, Portugal, to
develop automated tools that can assess and eventually forecast space
weather.

The Space Environment Information System for Operations (SEIS), now in use
at ESOC, has been tracking this month's solar activity based on data
gathered from numerous participating ground observatories as well as
spacecraft including Integral, Envisat and XMM-Newton, NASA's GOES
(Geostationary Operational Environmental Satellite) spacecraft.

"By monitoring reports generated by SEIS, we can estimate when solar fluxes
will reach the Earth, which can vary from a few hours to a few days from the
time of a solar flare," says Federico Di Marco, a flight engineer working on
Integral, the reference mission for the new SEIS tool.

His colleague Orlane Bergogne, also on the Integral team, produces a
Radiation Assessment generated by SEIS, showing X-ray and particle fluxes
for the month of December."

"The current solar activity actually began on 5 December, and we could
already see effects on Integral on 6 December. Eventually, we aim to develop
SEIS into a tool that can issue warnings and alerts to any mission operator,
which will be particularly valuable to spacecraft that don't have their own
radiation sensors on board," she says.

The Sun's active week

As reported on the SOHO mission site, the Sun unleashed a large (X-3 class)
solar flare this week on 13 December 2006, along with a coronal mass
ejection that headed towards Earth. Solar flares are classified as A, B, C,
M, or X, with the "X" category ranked as the strongest, based on peak flux,
or particle density.

The source of this week's eruptions was the very active sunspot region 930.
A shower of high-energy particles appeared as specks and white streaks on
the imagers aboard SOHO; the CME particles travel at speeds of up to several
thousand kilometres per second.

When the charged CME particles arrive at Earth, they can cause a variety of
disruptions, affecting communication and navigation networks, telephone
systems and broadcasts.

On 14 December, China's People's Daily reported widespread disruption of
shortwave radio communications in China on Wednesday morning. Astronauts on
board the International Space Station slept in protected areas of the
station as a precaution.

In October 2003, a solar flare forced Japan's Data Relay Test Satellite
(DRTS), also known as Kodama, into safe mode.

Further information:

European Space Agency ESA/ESOC
Corporate Communications Office
Tel +496151-90 2861

More information ...

* Spacecraft Operations
http://www.esa.int/spacecraftops/index.html

More news

* NOAA tracking space weather event
http://www.noaanews.noaa.gov/stories2006/s2758.htm
* See Mercurys silhouette with SOHO
http://www.esa.int/esaCP/SEMPIC0CYTE_index_0.html
* European expertise helps to view the Sun in a new way
http://www.esa.int/esaCP/SEMGJ6PFHTE_index_0.html

Related links

* SOHO and space weather
http://sohowww.nascom.nasa.gov/spaceweather
* ESA Space Weather
http://www.esa-spaceweather.net/index.html
* Coronal Mass Ejections
http://solarscience.msfc.nasa.gov/CMEs.shtml
* Envisat overview
http://www.esa.int/esaEO/SEMWYN2VQUD_index_0_m.html
* Cluster overview
http://www.esa.int/esaSC/120383_index_0_m.html
* Integral
http://www.esa.int/SPECIALS/Integral/index.html

[NOTE: Images supporting this release are available at
http://www.esa.int/esaCP/SEMB49QJNVE_index_1.html ]