Category Archives: photography|quirky

Return of the Afternoon Sun

Sunset from the Chumash Trail, Simi Valley, California.

Those of us in the northern hemisphere that enjoy afternoon daylight are celebrating the passing of the dank days of Autumn when sunset occurs the earliest in the day. Depending on your location, the amount of afternoon daylight may already be increasing — be it ever so modest.

According to the Astronomical Applications Dept. of the U. S. Naval Observatory, in Los Angeles that day is today, December 11, when the sunset shifts from 4:44 p.m. to 4:45 p.m.

The more northerly your latitude, the later the date. In Miami it was back on December 4, and in Seattle it will be on December 18. In Anchorage it won’t be until December 20. Barrow, Alaska won’t see a sunset (or sunrise) until January 23!

You can check your city’s sunset times using the USNO Sun or Moon Rise/Set Table.

Fox Mountain Frost

Hollow columnar hoarfrost deposited on leaves and twigs on Fox Mountain in the San Gabriel Mountains, near Los Angeles.

When I see crystals of hoar frost sparkle in the Winter sun it triggers a child-like awe. On Sunday’s Condor Peak Trail Run, several sections of trail glittered as we ran into a low morning sun. On the cold east face of Fox Mountain, a fine, needle-like frost coated the edges and surfaces of leaves and twigs that had collected in pockets on the steep slope.

Digitally magnifying a small section of a 10 Mp image revealed that the frost is comprised of  hollow columns, and further magnification shows that the columns are hexagonal, with lengthwise facets.

This type  of frost – hollow columnar hoarfrost – is described in STUDIES OF FROST AND ICE CRYSTALS by W.A. Bentley, in the Monthly Weather Review, Volume 35, Issue 9 (September 1907), pp. 397-403. Here is an excerpt:

“When formed in the open, they are essentially mild-weather types. They are most common to early autumn and late spring, and the hoarfrost that collects upon the plants and grasses during the so-called destructive frosts at those dates is almost invariably of this type. Hoarfrost deposits of this character form in the open during calm, clear nights when the surface air temperatures range from 56 degrees to 40 degrees at nightfall, and from 33 degrees to 25 degrees during the latter part of the night or early morning.”

Here is a graph of weather data recorded by the Mill Creek (ANF) RAWS on December 1 and December 2. The elevation of the station is 3510′ and it is about 8.5 miles from Fox Mountain (5033′). Parameters graphed are the hourly average wind speed, air temperature, fuel temperature, relative humidity, and dew point.

At Mill Creek the fuel temperature dropped below the frost point at 10:00 p.m Saturday, and did not exceed the frost point again until 8:00 a.m Sunday. For a 5 hour period from 2:00 a.m. to 7:00 a.m. the mean air temperature was 30°F-31°F and the fuel temperature was 22°F-23°F — suggesting strong radiative cooling. Similar conditions probably produced the frost on Fox Mountain.

Comet Holmes 17/P

Image of Comet Holmes 17/P taken in the light pollution of the San Fernando Valley, near Los Angeles, on November 13, 2007.

Image of Comet Holmes 17/P taken in the light pollution of the San Fernando Valley, near Los Angeles. It was photographed through the eyepiece of a 5 in. telescope (SCT) using one of my “running” cameras — a 10 Mp compact digital.

An exposure of 60 seconds was used. The raw format image was pushed 2.5 stops and the tone curve adjusted in Adobe Camera Raw to bring out detail in the diffuse outer coma of the comet. The image was flipped so that it is not reversed and is upright.

The comet’s nucleus is at about 8:00 o’clock, near the head of the more dense and bright inner coma. A hint of a tail can be seen projecting in the 2:00 o’clock direction. The tail of the comet isn’t more obvious because from Earth we’re seeing the comet almost head-on.

This illustration, generated using Starry Night Pro, shows the position of Comet Holmes 17/P on 11/13/07 – beyond the orbit of Mars – and its relationship to the Earth, Sun and the plane of the solar system. An orbit visualization and much more info is available on the Comet 17P/Holmes page on TheSkyLive.

Search Comet Holmes 17/P on Google for more info.

Milkweed Bug Nymphs

Large milkweed bug nymphs on a narrow-leaved milkweed seed pod.

The bright orange-red coloration of these immature large milkweed bugs (Oncopeltus fasciatus) is a warning to predators that they taste bad. Like monarch butterflies, they concentrate foul-tasting compounds from the narrow-leaf milkweed (Asclepias fascicularis) in their bodies.

Following several instars (molts), the nymph is transformed into the adult insect.

The photograph is from a run at Sage Ranch on July 23, 2007.