June 26, 2019

Astro-Vid Of the Week: Remembering the Halloween Flares of 2003

The Sun unleashes an X-Class flare on October 28th, 2003 as seen in UV.

(Credit: NASA/SOHO).

Our nearest star gave us a scare a decade ago this week. Back in 2003, none of us knew what Facebook or YouTube was, and most of us were still using ye’ ole message boards and chat rooms to discuss such seminal arguments as Kirk vs. Picard.

Sol was also just coming off of its peak for Cycle #23, and still had a trick or two up its sleeve. The action began with an X-ray Class X17.2 flare on October 28th, 2003. [Read more...]

03.03.11: The Riddle of the Blank Sun: Solved?

Researchers At the Indian Institute of Science and Education and the Harvard-Smithsonian Center for Astrophysics may have shed light on an enduring mystery from the past decade. In an article due to be published today in Nature, Dibyendu Nandi and co-author Andre Munoz-Jaramillo have come up with convincing evidence as to why the past solar minimum of 2008-09 was such a persistent one. During this minimum, over 600 spotless days occurred, the most since the great minimum of 1913. As a result, the outer magnetic sheath of the sun that we reside in shrunk, the Earth’s upper atmosphere cooled due to lower ultraviolet levels and contracted, and an increase of cosmic ray activity was seen in the inner solar system. This subsequently affected the usual drag that is induced on satellites, slowing down the rate of orbital decay and causing a buildup of space junk… just what’s up with our nearest star?

Now, researchers have built a model of the solar interior that fits a description of what has actually occurred; and the trouble started back at the peak of cycle #23 with a speeding up of the “Great Conveyor Belt” of plasma in the suns interior. This magnetic dynamo sub-ducts sunspot activity towards the poles, only to have them “well up” as these conveyors turn in opposite directions in both hemispheres. Paradoxically, a slowing down leads to a relaxing and expansion of the belt, allowing magnetic activity to surface; speeding up meant the activity never had a chance to surface. Sunspot activity usually begins at high latitudes at the beginning of a cycle, a hallmark that the new cycle is indeed underway. As the sunspot cycle progresses, sunspot activity tends to progress to lower latitudes. The model suggested by Nandi and Munoz is built on the buoyant evolution of sunspots versus the interplay of the magnetic dynamo and the meridional flows in the solar interior. This theory may also explain two other lingering mysteries; why are sunspots never seen at polar solar latitudes? Does the sun have longer cycles juxtaposed over the known 11 year one, such as the 70 year cycle that occurred in the 17th century known as the Maunder Minimum?

Researchers will soon have a chance to put all of these models to the test. NASA’s Solar Dynamics Observatory is on solar vigil, and the twin STEREO spacecraft have reached a vantage point giving scientists 360° coverage of the Sun. Solar cycle #24 will see the sun scrutinized as never before. Even today, two new sunspot groups have emerged, and a large prominence looking like an acacia tree can be seen on the limb of the sun from Astroguyz HQ via our trusty PST… the approaching 2013-14 solar maximum may prove to mark a renaissance in solar science.