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The channel is an excellent and very open place for
everyone to join and discuss all things related to the aurora phenomenon.
It is open to both novices and seasoned aurora spotters. At times when
there is a lot of activity some questions are asked over and over, "is
there going to be northern lights tonight?" is just one of the many.
I hope you understand that just as you, the more experienced people are
also trying to enjoy the show, and are busy analyzing the incoming data
as well. Please make sure your question is not already answered in this
FAQ before asking.
This page is also available in Dutch.
Comments or suggestions?
Aurora related FAQ:
1. Will there be aurora tonight?
2. Bz? Bt? Velocity? What does all this data mean?
3. How do I photograph the aurora?
4. What causes the aurora?
5. Why are there different colors in the aurora?
6. How do I read / what is Canopus?
7. What is LASCO, and where can I find the data?
8. What is EPAM and where can I find it?
9. X Class, M Class Flares? What are they, and where can
I follow these events? SEC data.
10. Where can I find some online all-sky aurora cameras?
11. I want to download stuff!
12. Are there any good books available on this topic?
13. What are sunspots, and what role do they play?
14. What are coronal holes, and what role do they play?
15. What is the magnetosphere?
16. What's My Geomagnetic Latitude? And why is there a difference
anyway?
17. What is the auroral oval?
18. Where can I find out more about the weather.
19. What is the Van Allen Belt?
20. What are all the services that are available in the
channel?
IRC related FAQ:
0. What is IRC?
1. What is Undernet, and why is the channel hosted there?
2. How do I get on the #SpaceWeather channel?
3. No one seems to be talking, does this thing work?
4. How is the channel organized? Who is who?
5. Where can I learn more about IRC?
6. Crash course IRC commands.
7. Netiquette
8. What is a netsplit?
9. How to get on the channel using HydraIRC
10. Some pointers for mobile phone users
1. Will there be aurora tonight?
This is very difficult to answer, and a question we
might get once every few minutes when there is an active storm. The factors
if it is visible where you are are many. Location, latitude, light pollution
by moon or cities, clouds, etc. etc. Read the latest forecast notes on
http://www.spacew.com/. And understand
that the question when exactly it will start is asking when the rain will
start when rain is expected in the weather forecast. Rest assured, when
people see the lights, you definitely WILL hear about it on the channel!
2. Bz? Bt? Velocity? What does all this data mean?
These are all data which are being recorded by the ACE
spacecraft. ACE is situated between the sun and the earth on the spot
where the gravity from both are the same. This records specifics on solar
wind. Because it is so far away, it usually takes around 40 minutes before
a front detected by ACE impacts the earth. Some of the data contains:
- Bz is the magnetic orientation of the solar wind, the
further south, the better. As opposites attract it will enable to solar
wind to 'attach' to the earth's magnetic field which will enhance the
transfer from particles into the magnetosphere. With a northwards Bz
they will be repelled. Values of -20 and lower are preferred.
- Velocity, sudden strong increases indicate a shock
front arrival. Values of 650 km/sec and higher are good values.
- Density, the amount of particles per cubic centimeter.
The more the better. A value of 10 and higher are preferred.
You can follow the 2 hour graphs
here.
3. How do I photograph the aurora?
Please take a look here.
For some starting points on exposure times, check this
page. Also the information in the gallery for each photo on http://www.northern-lights.no/
and http://www.spacew.com/ is a good
source of information.
On this site we added a page
with tutorials on how to edit photos of the aurora. For tips on actually
shooting the aurora in the field you better check out one of the links
mentioned before.
4. What causes the aurora?
In a few lines: charged particles which have been emitted
from the Sun are carried by the solar wind. When those particles reach
Earth they can be guided by the magnetic field towards the polar regions.
When they descend down our atmosphere they collide with molecules from
gasses such as Oxygen and Nitrogen which is causing the visible phenomenon
we are calling the Aurora Borealis (or Australis if it happens in the
Southern hemisphere). For further reading on what aurora is, please look
here
and here.
5. Why are there different colors in the aurora?
Please read this
article.
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6. How do I read Canopus?
If you look at the map,
you can see a row of dots in Canada and USA. There the data is collected
for this graph. The map shows the auroral oval (point 17), the location
where visible aurora takes place. The brighter the oval, the better.
Remember you can see aurora a bit further south, just look northwards
low on the horizon.
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Canopus's "full oval"
versus rtAmie's more correct geographical representation
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North America however is about 6 hours away from
Europe, and substorms can be a very localized event. So if you are
*not* in North America you are better of using another resource,
such as rtAmie.
This map is compiled from satellite data and is showing the auroral
oval over a map of the northern hemisphere in red gradients. The
amount of red represents how strong the oval is, just like the 'the
whiter the better' at the Canopus graph.
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7. What is LASCO, and where can I find the data?
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A full halo
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LASCO is one of the instruments on the ACE spacecraft
(see point 2), and its imagery shows the outer regions of the solar
atmosphere. It is especially useful to study the coronal mass ejection's
and flares that take place, and to see whether they will be earth
bound. Ideally you will see a "full halo" where a CME will
be directed straight towards earth. You can find one of the graphs
here. |
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snow in LASCO
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Occasionaly you can see a 'snow-storm' in the LASCO
data, as shown on the right in the animation. This is caused by protons
from the sun wich are being accelerated to very high speeds by the
eruptions, and then hit the camera on the LASCO spacecraft. |
8. What is EPAM and where can I find it?
An increase of the EPAM
plot is a sign of an upcoming front. Usually you see the red line going
up steadily (with a few hicks here and there) up to preferably values
of up to 1.0E+05 to 1.0E+06. When the front arrives this value will suddenly
rise a good ammount, after which it will plummet down.
9. X Class, M Class Flares? What are they, and where
can I follow these events? SEC data.
A solar flare occurs when the energy stored in a twisted
magnetic field is suddenly released, usually from a sunspot (point 13).
With these flares x-rays intensify as well. Using the SEC
plots you can follow the sun's x-ray output which is classified as A,
B, C, M, or X class events, going up in this order. Upper M class and
X class events are especially interesting for the northern lights enthusiasts.
Using the LASCO imagery (point 7) you can determine if they are associated
with earth bound coronal mass ejection's.
10. Where can I find some online all-sky aurora camera's?
Some nice all-sky camera's are: Kiruna,
Sweden, Sodankyla,
Finland, Alomar,
Norway, Poker
Flat, Alaska
11. I want to download stuff!
Don't we all want to download cool stuff! There
is a lot of free information on the Internet. For the people who want
to dive more into the theory, I'm sure you know how to use Google and
find scientific documents in .pdf format you can print out and learn from.
If you want a program you can use to follow the latest
data, STD Aurora Monitor
is the small brother of SWIM.
It is a program that has a freeware version you can download and evaluate.
Although this particular version has some shortcoming and annoying bugs,
you can't beat anything that's for free!
Solar Weather
Browser is a freeware program from SIDC that you can use to browse
solar events. On selecting a date it will retrieve the information over
the Internet. Very handy to find back data about flares.
SOHO is an important spacecraft for us. One of the instruments
onboard is LASCO which importance to us is explained in point 7. And on
their website
you can download a complete CD-ROM which contains a lot of information
regarding the instruments on the spacecraft, as well as explanations on
the solar wind and the sun itself. Not to be missed! If you have a newer
version of Windows and the CD-ROM does not want to run, you might have
to set your virtual memory to exactly 4000MB.
12. Are there any good books available on this topic?
There are several books available on this subject. But
if you need a single book which is easy to understand for the layman without
any (astro-) physics background, then The
Aurora Watcher's Handbook is the book to get. It touches all subjects
that are of interest to anyone interested this field.
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13. What are sunspots, and what role do they
play?
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Typical MDI Sunspot image
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Sunspots are areas on the sun that are darker because
they are cooler then the rest of the sun's surface and they have specific
magnetic configurations. If the conditions are right, a sunspot can
cause an eruption we call a flare. These flares can be associated
with a CME (coronal mass ejection). It is the CME that causes the
aurora. Sunspots are referenced too with a 3 digit number. You can
view actual photos of the sun with the spots and their number at MDI
Sunspot ID.
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14. What are coronal holes, and what role do
they play?
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The famous "Rudolph
the Reindeer" coronal hole which appeared at Christmas
2003
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Coronal holes are areas on the sun that appear to
be dark. These areas are known to cause a high speed solar wind, and
as such can cause northern lights. They can be seen in
EIT284. More information about corona holes can be found here.
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15. What is the magnetosphere?
Please read this
article. A graph which is interesting to follow during the impact
of a shock front is this
one.
16. What's My Geomagnetic Latitude? And why is there
a difference anyway?
We have two poles. One pole is the geographic pole,
which is being used on maps. The other is the geomagnetic pole, and is
the pole where actually all compasses point out to. The auroral oval where
the visible lights are taking place is attached to the magnetic pole.
This is why as watchers, our magnetic latitude is more relevant then our
geographical one. Also, the magnetic pole is tilted a bit towards Canada,
this is why during storms aurora can be seen much further south in North
America (geographically spoken!) than in Europe. To know what your magnetic
latitude is, please visit these pages: North
America, Eurasia,
South
Africa & Australia, South
America.
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17. What is the auroral oval?
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The auroral oval
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The auroral oval is the oval which is located around the
magnetic poles where the aurora takes place. More information can
be found here.
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18. Where can I find out more about the weather.
No matter how strong the storm is, if there are clouds
covering your observing location: no show! Often weather forecasts on
the radio or TV can be a bit too vague or general. At such times it is
often best to check the available satellite data yourself, and see where
you need to be. Satellite loops enable you to anticipate where clouds
will move to the coming hours, and even an 20km ride can sometimes make
the difference of seeing the lights, or miss them due to clouds! Some
suggestions for online weather resources:
| Europe: |
Unibas
- predicted cloud coverage the coming few days each 3 hours.
Meteosat
loop - great for anticipating where clouds will move to the coming
few hours.
USAF
- 120 hour forecast loop.
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| North America: |
NOAA
Let us know any suggestions
you have.
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| Australia and New Zealand: |
Let us know
any suggestions you have.
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19. What is the Van Allen Belt?
The Van Allen Belt is situated as a torus around the
earth at the height of the equator (in the equatorial plane). It works
as a trap for high energy particles from the sun and cosmos, which if
filled to its maximum can be released in substorms to the earth's polar
regions where they will create aurora. They are called after James Van
Allen who discovered them. More information can be found here.
20. What are all the services that are available
in the channel?
Several services are available in the channel, some
fully automated, and some you can use with commands. The services with
commands are:
| .seen <nick> |
This will give you information on when
<nick> has been seen the last. You can optionally use wildcards
(*) for any variable parts of a nick.
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| .lastspoke <nick> |
This will give you information on when
<nick> has last said anything in the channel.
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| .data |
This will give the latest solarwind data
as compiled by SporadiX. This is compiled once every 3 minutes.
Occasionally our sources have a "no data" record for the
last minute. If that happens, SporadiX will use the second last minute,
and add ! in front of the data to indicate this has happened. Please
note that sometimes also the second minute data is unavailable! If
that happens then you will see !NA (also for any minutes after that). |
Fully automated services are notification of reports
available on the Internet. Currently we have the next services setup:
| Reports |
Each whole hour SporadiX checks the several
reports. If one or more of these have new versions, then SporadiX
will notify that each 15 minutes for the next hour. The reports being
checked are: From Solar Terrestrial Dispatch: CME
Impact Prediction, Middle
Latitude Auroral Activity Warning, Middle
Latitude Auroral Activity Watch, Low
Latitude Auroral Activity Warning, Low
Latitude Auroral Activity Watch, Major
Solar Flare Warning, Forecast
Notes, Daily
Summary Solar Activity - Today and finally Daily
Summary Solar Activity - Yesterday, and from SIDC the Presto
Alert.
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| SIDC Cactus CME detection |
The Cactus
software at SIDC is a CME tracking system that fully autonomous
detects CME events on the Sun. Each 15 minutes SporadiX is checking
whether this system has released a new report and if that report contains
a new CME event. If so, it will report that a new CME has been found
to the channel, it will also indicate if the Cactus software detected
a possible halo event.
Although the Cactus system is still quite experimental it is a fast
way of reporting new CME's so we decided to include it in our services. |
0. What is IRC?
IRC stands for Internet Relay Chat and is one of the
older protocols on the Internet. The protocol defines a set of rules that
creates a way for groups of users to chat with each other. As the protocol
is very open it allows us to integrate special features such as services
that display solar wind data, etc.
1. What is Undernet, and why is the channel hosted
there?
Undernet is one
of the biggest IRC networks. A network consists of multiple IRC servers
located all over the world which are connected to form a single network.
Users who are connected to the same IRC network can chat with each other
if they have joined a common channel ('channel' is the correct IRC terminology
for a 'chat-room').
The benefit of using an existing network is that we
do not have to maintain our own IRC server for this. Also, the servers
in use on Undernet are of high quality, and usually connected directly
on important backbones that tie the whole Internet together. It's wise
you pick a server geographically close to you, for an optimal speed.
2. How do I get on the #SpaceWeather channel?
First you will need some way to connect to Undernet.
On the Undernet website there is a web
chat page you can use if you prefer not to install an IRC program.
To get on our channel perform the next steps:
- Fill in your preferred nick in "Nickname".
Pick a descriptive nick, as no two people can use the same nick on the
network. Optionally fill in an alternative nick if this is going to
be the case.
- In the "Your Favorite Channel" fill in #SpaceWeather.
- In the "Channel" dropdown menu, scroll all
the way down and select "Another channel".
- From the server drop down, pick a option that is geographically
closest to you.
- Hit Connect! If all goes well you should be brought
to the #SpaceWeather channel in a few seconds.
If you prefer to have a real IRC program installed
on your own computer, then there are a lot of options. On Windows mIRC
is a very popular program, but not for free. HydraIRC
is a freeware program for Windows. If you prefer another client, or you
are using another operating system, this
page has a list of options.
For configuration of other programs to get on our channel,
please take a look at the documentation of the program of your choice.
In all cases pick an Undernet server (preferably the one geographically
closest to you), and once connected, join the #SpaceWeather channel. How
to get on the channel using HydraIRC, we made this FAQ
on this page.
3. No one seems to be talking, does this thing
work?
Activity on the channel can vary a lot depending on
a few factors. The most important is activity of the sun and the solar
wind, of course. During active storms you can be assured there will be
a lot of chatting about! Between storms the activity can from time to
time be really low. The channel will still however be available, and so
are the services we offer in the channel.
4. How is the channel organized? Who is who?
You will notice some people's presence is more prominent
than others. The people with an @-sign before their name in the nick list
are "channel operators". The task of these people is to keep
order in the channel, and maintain it in all its aspects. In case of problems,
talk to one of them, preferably one that seems active at the moment.
There are also bots (short for robots) active as channel
operators. The most important one is SporadiX. This bot has several services
available, such as notification of new available reports (forecasts, etc.)
and display of current solar wind data and new detected CME's.
5. Where can I learn more about IRC?
There are a lot of IRC related websites available, http://www.new2chat.com/
and http://www.irchelp.org/irchelp/new2irc.html
are good places to start.
6. Crash course IRC commands.
Point 5 will be of much bigger help, but we will list
a few of the most important commands here if you need a crash course:
| /nick newNick |
This will change your nickname. |
| /join #channelname |
This will join you in the given channel. |
| /part #channelname |
This will make you part the channel. |
| /query nick |
This will open a new window with the
person you gave as nick. The text in this window will only be visible
for you and the person you supplied the nick for. There is a maximum
of 2 people for this. For more, you will need to open a new channel. |
| /notice nick And some text |
A notice is handy for sending just a
few lines of text to a person if it needs to be done in private. Only
the person you supplied the nick for will be able to read this text.
Depending on the IRC program used it can be seen by the recipient
in the active window, or status window. |
| /whois nick |
Gives some information about the supplied
nick. |
| /quit and a short message |
This make your program stop the connection,
and display the optional message you supplied. |
7. Netiquette
A small word about using proper netiquette (etiquette
on the Internet). The channel can be very busy at times, and constantly
repeating yourself will not be appreciated at such times. Especially by
those who are online from the field with for example a mobile phone. Especially
during busy times: stay on topic, which will save a lot of unnecessary
text. DO NOT WRITE IN ALL CAPS, it is considered as shouting. Do not make
use of excessive colors, or scripts that give unnecessary colors and messages
in the channel.
8. What is a netsplit?
The Undernet IRC network consists of a large number
of servers all around the world that are connected to each other. From
time to time it can happen that the connection between two of such servers
has a temporary hiccup. The users on either side will see the users from
the 'other side' leave the channel with a message similar like this: ***
nick (ident@some.isp.com) Quit (*.net *.split)
If the netsplit occurs between the two servers connecting
both sides of the Atlantic Ocean, the number of users parting the channel
might be quite big. In most cases, the split will not take long, and you
should see the 'other side' joining back within a few minutes.
If you are on a single server that have been split off
the network, and it takes quite long, you can try another server to join
back with the others. Netsplits are a small annoyance in the use of IRC,
but the benefits, such as running our own bots which can display data,
greatly out benefit it.
9. How to get on the channel using HydraIRC
After you downloaded and installed the program, and
run it the first time, you will have to create a identity. Type in the
following information, ofcourse change to your preferred nickname, and
click the Add button:
After this you can click the connect button which you can
find on the iconbar on the top of the program. I have a red circle around
the icon on the next image:
In the following window, scroll down a little, and click
on "Undernet", and then the irc.undernet.org server, and then
click OK:
Now a new window will be opened, and the program will try
and connect to the Undernet network. This might take a few seconds. Once
connected a channel list window will be opened wich you can close, you
already know what channel you want to join! Type in the edit box of the
server window: /join #spaceweather And again
a new window will be opened, this time for the channel, congratulations,
you made it!
10. Some pointers for mobile phone users
If you are with a mobile phone in the field, we have
a secondary channel which might be interesting for you. On #spaceweatherdata
you will be unable to talk, but the bot will be there to regurally give
the latest data just as in the main channel. A good and cheap way to follow
the lastest data in the field, without the high costs of downloading any
graphs, or a lot of noise of the regular chat from the main channel you
would otherwise have to scroll through on your small window. The data
will also be updated faster then in the main channel.
If you need a java client for mobile phones, jmIrc
is a free option.
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