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Glendale App is the world's most accurate aurora alerting and forecasting app. Over 70,000 users.
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Noctilucent clouds are lit by sunlight in an area of the night sky called the Twilight Arc.
My twilight-arc tracker is constantly monitoring the position of the sun at your location and calculating the position and height of the twilight arc.
The centre of the twilight arc is at the sun's azimuth. The sun's elevation is its angle above (or below, if -ve) the horizon.
The 'Max Heights' are the maximum angles above the horizon that Noctilucent Clouds and Cirrus can be lit directly by sunlight.
NLCs are only visible when the sun is in a narrow range of angles below the horizon that are dependent on your latitude. The optimum times, when you have the highest chance of seeing them are shown.
They are much rarer than auroras, typically seen fewer than 15 nights per year. They are clearly visible by eye, even in towns and cities.
There is no way to predict noctilucent clouds. The trick is to look every night at the optimum times given on this app and you will get lucky.
Global, real-time tracking of auroral substorms is only possible due to some incredible organisations allowing me to access the live data from their magnetometer arrays.
I am indebted to the kindness and generosity of the Tromsø Geophysical Observatory, Swedish Institute of Space Physics, the US Geological Survey and the Finnish Meteorological Institute for letting me access their live data feeds.
I am also indebted to I.R. Mann, D.K. Milling and the rest of the CARISMA team for use of data from the Canadian magnetometer array. CARISMA is operated by the University of Alberta, funded by the Canadian Space Agency.
Mann, I. R., et al. (2008), The upgraded CARISMA magnetometer array in the THEMIS era, Space Sci. Rev., 141, 413–451, doi:10.1007/s11214-008-9457-6.
The headline figure -100 nT is the strength of the aurora in the sky right now, called the substorm strength.
Watch this number! You want it negative. The more negative it is, the stronger the aurora is at that minute. Falling is good, rising is bad. It tracks the strength of the actual aurora in the sky in real-time. It is the single most important number on the app and overrides all others.
When it says 'growth', the substorm is charging up like a battery. When it says 'expansion' that energy is being released as aurora. When it says 'recovery', the aurora will slowly begin to fade.
The trendline shows the changes in strength over the last hour. The line dropping sharply downwards is good. Rising is bad. The blue shaded area indicates the ambient level.
IMF tells us about the future, not the present. We use it to predict activity 1 to 3 hours from now.
The table shows an analysis of the interplanetary magnetic field in the 30 minute window that is currently arriving at Earth, together with windows either side of it. The 'percentage' figure indicates how negative the Bz was, the ideal is 100% negative.
If the 'now' and 'next' rows are both lit up, the substorm will continue if one is active or will start in about an hour if one isn't active.
If the 'next' row is not lit up, the activity will start to wane if a substorm is active but there can be an extra burst of activity, so wait an hour.
When a substorm is in its expansion phase all of these values are irrelevant to that substorm. Substorm strength overrides all other metrics.
The trendlines show the Bz and Bt that is arriving at Earth now (left) and as far into the future as it is possible to see, at L1 satellites (right). Bt is at the top, Bz in the middle and the optimum Bz at the bottom (black).
The middle line is the important one. You want it to be below the blue shaded (ambient) area and as close to the black line as possible.
This is the mean velocity, density and pressure of the solar wind that is currently arriving at the Earth. They don't really matter that much for aurora. IMF is much more important. A good IMF will lead to aurora even when speed and density are at ambient levels. We use solar wind data to look for space weather events that might bring us good IMF.
When a substorm is active, all of these values are irrelevant. Substorm strength overrides all other metrics.
When the IMF is strong and well-aligned, these values are irrelevant. IMF overrides solar wind speed & density.
The trendlines show the solar wind speed and density that is arriving at Earth now (left) and as far into the future as it is possible to see, at L1 satellites (right). The blue shaded area indicates the ambient level.
Coronal holes cause most of our auroras and they are regular, repeating on a 27 day cycle. Plasma from an Earth-facing coronal hole typically takes 3 to 4 days to reach us and spark auroras.
Flipping between the 'now' and '-27 days' tabs allows you to see how coronal holes have changed since their last rotation 27 days ago.
The '-4 days' tab allows you to see how the coronal hole looked when it was in the earth-facing position 4 days ago.
Solar imagery courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
Coronal Mass Ejections are bursts of plasma that sometimes erupt from sunspots during a solar flare. They can trigger the strongest auroras if they hit Earth.
You are looking for plasma surrounding more than 50% of the solar disk in this graphic (a partial halo). The ideal is a 'full halo', where plasma appears to surround the entire solar disk. It then takes 2 to 3 days for the CME to reach Earth.
Even when there appears to be an Earth-directed component or it looks like a direct hit, the CME can still miss completely or bounce off the Earth's magnetosphere. Don't get too excited until the app alerts that a shock has been detected!
Don't take any ETAs too seriously, either here or on other sites, as they are only a very rough guide.
CME data and graphics derived by Glendale App from solar imagery kindly provided by SOHO.
Solar flares from sunspots sometimes produce a CME which, if directed earthward, can cause strong substorms between two and four days after the eruption.
Most flares don't produce a CME and most CMEs miss the Earth, so don't get too excited about flares.
Flares are classed A, B, C, M or X with A being weakest and X being strongest. The number indicates how strong the flare was within its class.
After a flare, it can take several hours before imagery becomes available that enables us to determine whether there was a CME and whether that CME was Earth-directed. After a flare, keep checking the Coronal Mass Ejections panel for the latest updates as imagery arrives.
The image shows the active region that was the source of the most recent solar flare, highlighted with a yellow circle. When there have been no recent flares it shows the latest image of the solar disk.
The sun spins on its axis effectively every 27 days, which means that coronal holes and active regions giving us auroras today can rotate back around again in 27 days time, giving another show.
These are the dates when solar wind streams that gave us good auroras will rotate around again. There is no guarantee that the coronal holes that caused the substorms on the previous rotation won't have closed but they also may have got larger. You can only use these as a guide but this is the most accurate long-range forecast for the UK, Ireland, Iceland, Scandinavia, North America and Australasia that you will find anywhere in the world.
It is essential to check the coronal holes panel, as we get closer to the dates that interest you, to confirm the current status of the hole that caused the activity, as it might have closed. This forecast should only be used for dates 9 to 27 days in the future.
This forecast is based on my own data collected in the UK and is valid worldwide. The more negative the figure, the stronger the aurora could be.
Dates that are coloured black are uncertain. Dates shown in colour are more likely. Dates that are missing have no predicted activity.
* You need to register to view the full 28-day forecast.
If you have forgotten your password, an email will be sent to your registered email address with a link to reset it. Click 'Reset Password' button and follow the instructions in the email to log back in.
If you have forgotten what your own name is, an email can be sent to your registered email address with a reminder. Click 'Send My Name' button and a reminder will be sent to you.
Entering your details here will allow you to make instant, live, aurora reports to let others know what the current situation is where you are. You will also be able to see reports from other users, access all features of the app and see the live data in real-time.
Enter the exact same details on all devices where you use the app to synchronise your history and reports across them all.
If you work as an aurora tour guide, researcher, scientist or are an admin on an aurora facebook site you can enter those details and they may be shown to other users.
Your actual name, your actual email address and the name of your nearest town/village are required to use this app. Only your first and last name are required. Abuses will result in the account being de-activated. This includes nick-names, truncation, obfuscation, business names, junk, burner emails, emails that bounce, etc.
This app collects sighting reports you make for purposes of scientific research, to improve the accuracy of aurora forecasting and for alerting users when the aurora is active.
Your personal data is not shared with any other organisations or third parties.
You will not be spammed. You may be contacted about interesting reports you have made, problems you are having with the app or security/authentication issues.
This app only uses essential cookies.
The commonest reason for your account being blocked is that you have a mistake in your email address. If the account activation email bounces your account will automatically be blocked. Check your email address very carefully. It may also be due to your name failing to meet the account rules.
The commonest reason that you haven't received an activation code is that you have a mistake in your email address. Check your email address very carefully. If you are certain the email is correct then it is most likely your spam filter, to unblock this email me from the email account you are registering with and request a code.
Your phone is android and is capable of receiving alerts but you need to install the Chrome app and make it your default web browser.
To install this web app on your device:
Go to aurora-alerts.uk.
Press SHARE button in Safari (NOT 'share' in the app).
Add to Home Screen.
Add (top right).
Open Chrome or Firefox.
Go to aurora-alerts.uk.
Click the red 'install the app' button.
Open the Chrome App.
Go to aurora-alerts.uk.
Click three vertical dots icon (top right).
Add To Home Screen.
Click 'Enable Alerts'.
App installed and tile added.
The basic alerts are push notifications that the app sends automatically when it detects that an aurora is developing. An 'onset' alert is sent first as a warning that an aurora is starting, followed by yellow, amber, red, major, severe and extreme alerts as activity develops. Your device will receive these even when the app is not running.
The 'Expansion Alarm' is designed for desktop users. If you leave the app running permanently on your PC, the app will start bleeping as soon as it detects a substorm heading into expansion phase to give you time to head out and catch it at its peak.
'Activity Alerts' are notifications that can be set to 'ping' your device only when the app is running. These occur much more frequently than the basic alerts. They alert you to all thresholds being crossed, auroras being reported by users and photos being uploaded. These are great for users of desktop PCs who want to keep constantly updated on the current aurora situation.
The plot shows the substorm strength over the last 24 hours, which allows you to see the periods when the aurora was at its best.
The more negative the figure, the stronger the aurora was.
These graphs are deliberately produced 5+ minutes behind real-time. Use the Substorm Panel above for aurora-hunting.
These graphs allow you to verify the accuracy of this app by comparing the times of your best photos against the substorm strength the following day. You will see that your best photos were taken precisely on the best drops. Remember that the graphs are in UTC time, not your local time.
The plot shows the IMF Bt (black) & Bz (red) over the last 24 hours, which allows you to see the periods when the IMF was strongest.
The pale green line shows the By.
The plot shows the clock angle (θ) over the last 24 hours, which allows you to see the periods when the IMF was best aligned.
The plot shows the solar wind speed & density over the last 24 hours.
Ideally what you are looking for on the stackplot are dips of >200nT on the right-hand side of the line labelled 'and' or any of the lines below it.
Stackplot courtesy of the Tromsø Geophysical Observatory.
Glendale App was created by Andy Stables of the Glendale Skye Auroras Facebook Page to make it easy for people to photograph the Aurora Borealis. It is the result of research carried out on a daily basis since September 2012 in the Isle of Skye.
The world-leading accuracy of the app is only possible due to the generosity of the Tromsø Geophysical Observatory, the Swedish Institude of Space Physics, the US Geological Survey, the Finnish Meteorological Institute and the CARISMA team in allowing me to access the live data feeds from their entire magnetometer arrays around the northern hemisphere.
The wonderful icons for the tiles, badges and logo were the work of Andrew Liley from Portree.
The Iceland Version of the App was only made possible thanks to many hours of detailed observation and recording by Caroline Weir from Reykjavik, who runs the Aurora Iceland Facebook Group.
Read the full behind-the-scenes story of Glendale App here.
Europe, Canada & Oceania Maps by vemaps.com.