This spectacular north looking view of south Greenland (62.0N, 46.0W) shows numerous indentations along the coastline, many of which contain small settlements. These indentations are fiords carved by glaciers of the last ice age. Even today, ice in the center of Greenland is as much as 10,000 ft. thick and great rivers of ice continuously flow toward the sea, where they melt or break off as icebergs - some of which may be seen floating offshore.
South Greenland, North Atlantic Ocean
This north-looking view of southwestern Greenland was taken in November, 1994, and shows numerous indentations, many of which contain small settlements. These fjords were carved by the glaciers of the last ice age 10,000 years ago. Even today, the ice in the center of Greenland is nearly 3,500 meters (11,000 feet) thick and great rivers of ice continuously flow down toward the sea, where they melt or break off as icebergs. Some Icebergs exceed the size of small islands, weigh several million tons, and rise several hundred feet above the sea surface. Cape Farewell is visible toward the bottom right of the view. Julianehab Bay and the Bredev fjord can be seen toward the center of the photograph. Godthab, the main settlement on Greenland, is barely visible to the north of the Frederikeshabs Icefield near the left center of the view.
Greenland as seen by the STS-66 shuttle Atlantis
ISS038-E-047389 (14 Feb. 2014) --- This panoramic image, which shows parts of Chile and Argentina, and which was exposed with an 80mm lens from the International Space Station (ISS),  captures Tierra del Fuego and Cape Horn.  Represented here is the southernmost tip of South America (left), with the Atlantic Ocean in the foreground and the Pacific Ocean across the top of the image.  Crews on the orbital outpost seldom see Cape Horn in such clear weather. Shortly after this image was taken, the cloud mass approaching from the Pacific Ocean completely obscured the landscape from the station’s view. In this stormy part of the world, ships avoid the heavy seas around exposed Cape Horn and use the protected Strait of Magellan (lower right) on the inshore end of Tierra del Fuego.  A small white ice field on the highest parts of Tierra del Fuego (center right) includes Mount Darwin, situated within Chile’s Agostini National Park. The ice field can be imagined as greatly expanded during the geologically recent ice ages, covering an area greater than the land area shown in this view. The heavily indented shape of the fiord coastline and the lake depressions (center and lower right) were carved by the downhill movement of these vanished glaciers, according to NASA scientists.
Earth Observations taken by Expedition 38 Crewmember
This pair of images illustrates the ability of multi-parameter radar imaging sensors such as the Spaceborne Imaging Radar-C/X-band Synthetic Aperture radar to detect climate-related changes on the Patagonian ice fields in the Andes Mountains of Chile and Argentina. The images show nearly the same area of the south Patagonian ice field as it was imaged during two space shuttle flights in 1994 that were conducted five-and-a-half months apart. The images, centered at 49.0 degrees south latitude and 73.5degrees west longitude, include several large outlet glaciers.  The images were acquired by SIR-C/X-SAR on board the space shuttle Endeavour during April and October 1994. The top image was acquired on April 14, 1994, at 10:46 p.m. local time, while the bottom image was acquired on October 5,1994, at 10:57 p.m. local time. Both were acquired during the 77th orbit of the space shuttle. The area shown is approximately 100 kilometers by 58 kilometers (62 miles by 36 miles) with north toward the upper right. The colors in the images were obtained using the following radar channels: red represents the C-band (horizontally transmitted and received); green represents the L-band (horizontally transmitted and received); blue represents the L-band (horizontally transmitted and vertically received). The overall dark tone of the colors in the central portion of the April image indicates that the interior of the ice field is covered with thick wet snow. The outlet glaciers, consisting of rough bare ice, are the brightly colored yellow and purple lobes which terminate at calving fronts into the dark waters of lakes and fiords. During the second mission the temperatures were colder and the corresponding change in snow and ice conditions is readily apparent by comparing the images. The interior of the ice field is brighter because of increased radar return from the dryer snow. The distinct green/orange boundary on the ice field indicates an abrupt change in the structure of the snowcap, a direct indication of the steep meteorological gradients known to exist in this region. The bluer color of the outlet glaciers is probably due to a thin snow cover. A portion of the terminus of the outlet glacier at the top left center of the images has advanced approximately 600 meters (1,970 feet) in the five-and-a-half months between the two missions. Because of the persistent cloud cover this observation was only possible by using the orbiting, remote imaging radar system.  http://photojournal.jpl.nasa.gov/catalog/PIA01778
Space Radar Image of Patagonian Ice Fields