eiscat radar school 23.8.2005, kiruna, sweden aurora and auroral studies with is radars kari kaila...

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Eiscat Radar School 23.8. 2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

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Page 1: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurora and Auroral Studies with IS radars

Kari Kaila

University of Oulu

Department of Physical Sciences

Page 2: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Introduction

Page 3: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: Where the name comes?

• Aurora is latin and means dawn. It looks like dawn is approaching after dark night

• In many languages it means Northern light

• Aurora borealis is Northern dawn and Aurora Australis Southern Dawn

• In Finnish language it is Revontulet and means Fox fires

Page 4: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: What they are?

• Aurorae are luminous phenomenon which are seen during dark nights

• They were mysterious phenomena, which have been observed couple of thousands of years

• Mostly they are calm and quiet

• Sometimes they are very vivid

Page 5: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 6: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 7: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: How do they look like?

• Most often they can be seen east-west directed arcs low in the north

• They are pale or gray surfaces in the sky

• In the pre midnight sector they move typically very slowly southward

• When getting brighter, the greenish colour becomes clear visible

Page 8: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: How do they look like?

• Most common forms are quiet arcs and luminous diffuse light in the north

• Sometimes the quiet arc starts to disturb. It becomes a folded band.

• Vertical rays may appear in the arc or band and clear motion can be seen in the form.

• All the forms move southward

Page 9: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: How do they look like?

• Suddendly the southernmost arc stops, fades and the a beautiful display starts: auroral breakup or auroral substorm

• The southernmost arc becomes brighter and long rays appear on it. Soon new bright arcs and bands appear and different colours are visible and within minutes the sky is full of different bright auroral forms.

Page 10: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 11: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: Where they are?

• They can be seen close to the poles, in north and in south

• At the poles they are rather rare

• They are most commonly observable about 2000 km from the magnetic poles

• When passing the maximum region, they became again rare closer to the Equator

Page 12: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 13: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 14: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 15: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 16: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 17: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 18: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Aurorae: Connection to the Sun?

• The appearance of aurorae follows the periodes of the Sun

• Aurorae appear more often when the sun is active. The Sun has 11 years cycle and so do the aurorae have.

• The Sun rotates around its axis in about 27 days. If bright auroral display may repeat again after 27 days.

Page 19: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 20: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 21: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 22: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 23: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Instruments:satellites, photometers,

cameras

Page 24: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 25: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 26: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 27: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 28: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 29: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

DMSP-F13 F13199705102347.6.ols.tir.gif

Page 30: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 31: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 32: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 33: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 34: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 35: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Page 36: Eiscat Radar School 23.8.2005, Kiruna, Sweden Aurora and Auroral Studies with IS radars Kari Kaila University of Oulu Department of Physical Sciences

Eiscat Radar School 23.8.2005, Kiruna, Sweden

Polar images

• This image has been acquired with the Earth Camera that is one of three cameras in the Visible Imaging System (VIS). The design and assembly of the VIS was performed by the VIS team at The University of Iowa. The VIS is one of twelve instruments on the Polar satellite of the NASA Goddard Space Flight Center.

• The Principal Investigator is Dr. L. A. Frank and the Instrument Scientist and Manager is Dr. John B. Sigwarth.