KenMankoff

The role of Pine Island Glacier ice shelf basal channels in deep-water upwelling, polynyas and ocean circulation in Pine Island Bay, Antarctica

The role of Pine Island Glacier ice shelf basal channels in deep-water upwelling, polynyas and ocean circulation in Pine Island Bay, Antarctica

Several hundred visible and thermal infrared satellite images of Antarctica’s southeast Amundsen Sea from 1986 to 2011, combined with aerial observations in 2009, show a strong inverse relation between prominent curvilinear surface depressions and the underlying basal morphology of the outer Pine Island Glacier ice shelf. Shipboard measurements near the calving front reveal positive temperature, salinity and current anomalies indicative of melt-laden, deep-water outflows near and above the larger channel termini. These buoyant plumes rise to the surface and are expressed as small polynyas in the sea ice and thermal signatures in the open water. The warm upwellings also trace the cyclonic surface circulation in Pine Island Bay. The satellite coverage suggests changing modes of ocean/ ice interactions, dominated by leads along the ice shelf through 1999, fast ice and polynyas from 2000 to 2007, and larger areas of open water since 2008.

@article{Mankoff:2012The-role,
	Title = {{The role of Pine Island Glacier ice shelf basal
                  channels in deep water upwelling, polynyas, and
                  ocean circulation in Pine Island Bay, Antarctica}},
	Author = {Kenneth D. Mankoff and Stanley S. Jacobs and
                  Slawek M. Tulaczyk and Sharon E. Stammerjohn},
	Journal = {Annals of Glaciology},
	Number = {60},
	Volume = {53},
	Year = {2012},
        DOI = {10.3189/2012AoG60A062}}

Pine Island Glacier and Pine Island Bay

Pine Island Glacier and Pine Island Bay

Pine Island Bay in the southeast Amundsen Sea, Antarctica, on 16 Nov 2008. Upwelling, melt-laden outflow plumes emerge from beneath the adjacent Pine Island Glacier ice shelf (top center) and mix in the bay waters. Warm red colors show sea surface temperatures more than a degree warmer than the near-freezing dark blue color. Cyclonic circulation in the bay is framed by the ice shelf, land ice and sea ice, in gray-scale with the darker shades colder. Landsat Enhanced Thematic Mapper Plus image, thermal infrared (channel 6H), subset of scene #LE72331132008321EDC00.

@article{Mankoff:2012The-role,
	Title = {{The role of Pine Island Glacier ice shelf basal
                  channels in deep water upwelling, polynyas, and
                  ocean circulation in Pine Island Bay, Antarctica}},
	Author = {Kenneth D. Mankoff and Stanley S. Jacobs and
                  Slawek M. Tulaczyk and Sharon E. Stammerjohn},
	Journal = {Annals of Glaciology},
	Number = {60},
	Volume = {53},
	Year = {2012},
        DOI = {10.3189/2012AoG60A062}}

YAGEL – Multiple Balloons on Mars

I’m releasing Yet Another Google Earth Layer, this one featuring some more KML tricks and hacks pushing Google Earth to do things that Google does not officially support: multiple placemark description balloons visible at once.

Download: Mariner Mars 1971 (MM71) Ultraviolet Spectrometer (UVS) Data in Google Earth. This is a work in progress as part of a Planetary Data Restoration Project at the Laboratory for Atmospheric and Space Physics and as such the data is not finalized and is subject to change.

The data comes from the Ultraviolet Spectrometer on the Mariner Mars 1971 spacecraft, and had previously been processed for the Albatross software tool back in 2002. Neither Google Earth nor its predecessor KeyHole, nor even KML, existed back in 2002, and the data needs to be accessible in a more modern and accessible visualization tool (Google Earth) in order to remain useful.

The footprints are where the instrument was looking. In each of these regions a spectral range from 2107 to 3497 Ångströms was sampled, and the spectra are visible in both the hacked multi-balloon display, and in the more detailed official Google Earth balloon visible by clicking on the footprint. Each footprint is colored, both in the map view and in the sidebar, by the response at 3049 Å, which is roughly where the ozone signal is. For more information on the data and science see the references listed at the end of this post.

Previously I implemented vertical data “curtains” in KML, useful for oceanographic transects, seismic lines, spacecraft looking down through the atmosphere in profile (as opposed to a 2D surface image), or any other vertical data. Along with vertical data (solved) and subsurface data (no known work-around), another major limitation of Google Earth is that only one description balloon is allowed to be visible at a time. However, Google Earth does support multiple placemarks (by default yellow pushpins in Google Earth, or red pins in Google Maps). The hack to get multiple balloons visible at once is to make custom icons that look like balloons and then use them in place of the default icons. If this technique is used it is advised to implement various other KML features to make the balloons only appear in certain views and therefore avoid overwhelming the viewer. I’ve used both the TimeStamp and the Level of Detail features to limit when the icons appear.

@article{barth1974atmosphere,
  title={{The atmosphere of Mars}},
  author={Barth, C.A.},
  journal={Annual Review of Earth and Planetary Sciences},
  volume={2},
  number={1},
  pages={333--367},
  year={1974},
  publisher={Annual Reviews}
}

@article{barth1971mariner,
  title={{Mariner 6 and 7 ultraviolet spectrometer
                   experiment: Upper atmosphere data}},
  author={Barth, CA and Hord, CW and Pearce, JB and
                 Kelly, KK and Anderson, GP and Stewart, AI},
  journal={J. geophys. Res},
  volume={76},
  year={1971}
}

Mars Geology

Data from the U.S.G.S. PIGWAD site converted to display in Google Mars. View the KML layer or the legend (also available through the layer).

Mars Geology

@conference{skinner2006digital,
  title={{Digital renovation of the atlas of Mars 
         1: 15,000,000-scale global geologic series maps}},
  author={Skinner Jr, JA and Hare, TM and Tanaka, KL},
  booktitle={37th Annual Lunar and Planetary Science Conference},
  volume={37},
  pages={2331},
  year={2006}
}

Earthquakes

I came across a database of earthquakes from 1960 to almost present. I converted it from the existing form to KML so it can be seen in both Google Earth and Google Maps. Both views incorporate a temporal component.

For the Google Earth view, magnitude as been encoded as pin size and depth has been encoded as height above the Earth. A few interesting regions where the deep quakes occur, such as east of the Andes, pop out.

Earthquakes

Iceland’s Root

Iceland's Root

Image appears to be related to Wolfe et al. (1997). Also available in Schubert and Turcotte below the discussion. Image found at LDEO.

Pine Island Glacier Publication TimeMap

In which I present a rough geo-spatial-temporal map of Pine Island Glacier (PIG) publications.

Geo-spatial-temporal time-map of Pine Island Glacier (PIG) publications

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GISTEMP.StationData

NASA GISS has recently announced another year of the surface temperature trends. Last year, 2009, tied for the 2nd warmest year on record, and the past decade (January 2000 to December 2009) was the warmest on record.

I took the time this weekend to re-create a Google Earth layer showing these data. This visualization allows you to see a broad geospatial overview, and then select any particular location and see both long-term trends and even the data point for each individual month.

Download (330K)

GISTEMP.StationData

GISTEMP.StationData