What Does Unusual Auroral Activity Mean in Astronomy?

  • Context: Undergrad 
  • Thread starter Thread starter CallMeSusan
  • Start date Start date
  • Tags Tags
    Activity
Click For Summary
SUMMARY

The discussion focuses on unusual auroral features observed by the DMSP-F6 satellite on January 10 and 11, which included a shift in the most active auroral region to the morning sector and a large number of sun-earth aligned arcs. The analysis indicates that these anomalies are attributed to significant changes in the Interplanetary Magnetic Field (IMF), specifically large BY and positive Bz components. The conversation also touches on the implications of these observations for satellite communications and the current state of the solar cycle, suggesting that such unusual auroral activity may become more common due to the weak Maunder cycle.

PREREQUISITES
  • Understanding of the Interplanetary Magnetic Field (IMF)
  • Knowledge of auroral phenomena and their characteristics
  • Familiarity with satellite observation tools like DMSP-F6
  • Basic concepts of solar cycles, particularly the Maunder cycle
NEXT STEPS
  • Research the effects of the Interplanetary Magnetic Field on auroras
  • Study the relationship between solar cycles and auroral intensity
  • Explore satellite data analysis techniques for auroral observations
  • Investigate the implications of space weather on satellite communications
USEFUL FOR

Astronomy enthusiasts, space weather researchers, satellite communication engineers, and anyone interested in the dynamics of auroras and their relation to solar activity.

CallMeSusan
Messages
2
Reaction score
0
Hi,

I am a newbie trying out astronomy after two decades of politics, but I was hoping if someone could help translate the following statement for me (I am not a student, so your not answering an essay question or anything);

We report unusual auroral features observed by the DMSP-F6 satellite on January 10 and 11. These features include the shift of the most active region to the morning sector, the shift of the polar cap center toward the evening sector, a large number of sun-earth aligned arcs and the oval-shaped diffuse glow without bright oval arcs. The simultaneous magnetic field observations by the ISEE-3 and IMP-8 satellites, together with a simple magnetospheric modeling result, suggest that the unusual features result from both the unusually large BY and a large positive Bz component of the IMF.

The italic/bold section confuses me somewhat. The answer (the last sentence) doesn't really explain it.
 
Astronomy news on Phys.org
Welcome to Physics Forums.

A page that explains the Interplanetary Magnetic field

http://www.spaceweatherlive.com/en/help/the-interplanetary-magnetic-field-imf

The aurora we see on Earth is the result of "stuff" that is ejected from the sun interacting, way up high, with atoms in Earth's atmosphere. The atoms become excited and give off light. The "stuff" is made of charged particles. The particles, because they have a charge, are affected by Earth's magnetic field and the IMF.

What the bold part talks about, in part, is the areas of the auroral glow are not where they usually are. The morning sector is the area where sunrise is happening on Earth -- looking down onto the North (or South Pole). The polar sector is directly over the pole. You can guess what the evening sector is.

The auroral display has features like arcs, glow, striations. If you have not been to the far North or South you probably have not seen them. They are wonderful.
http://en.wikipedia.org/wiki/Aurora_(astronomy )

The bold section is talking about displays that are out of the ordinary and are in places where they may not normally be seen.

The Bx, By, and Bz are vector components (think of a vector as direction and velocity like your car on the highway) that make up the IMF. The vector has 3 dimensions: (B)x,(B)y and (B)z. The article is saying that changes in magnitudes of Bz and By caused the unusual aurora.

Space Weather (the charged particles, and the IMF) is very important to satellite communications.
 
Last edited by a moderator:
Thanks Jim, I appreciate the clarity. I understand that the date of the journal article is quite old (1983) - would you know, by any chance, whether activity such as this often occurs, or was it quite unique for that day/moment (as in the shift of the most active region to the morning sector etc)? I only ask this because I am confused as to why this is "unusual".
 
Last edited:
Space Weather is a fairly young, evolving science, so some of their observations and goals have been moving targets, so to speak. I do not know whether this was a one time anomaly or not. As a guess I would say no.

The current Maunder cycle -- 24 -- (sunspot cycles influence aurora intensity) is weak, so if there are going to be anomalies, this may be a chance to see them. According to the report:

http://solarscience.msfc.nasa.gov/SunspotCycle.shtmlSunspot numbers and solar output appear to be declining. The report makes an analogy between the current trend and sunspot numbers in the late 17th Century.
 
Last edited:

Similar threads

  • · Replies 13 ·
Replies
13
Views
6K