November 8, 2018 Page 5
BLT Shrimp Roll
Recipe provided by Brandpoint • Servings: 6 • Time: 11-20 minutes
Ingredients
• 6 Sara Lee Artesano Bakery
Rolls
• Juice of 1 lemon (about 2 tablespoons)
• 3/4 cup mayonnaise
• 1 tablespoon white wine vinegar
• 1 teaspoon Dijon mustard
• 1/2 teaspoon sugar
• 1/2 teaspoon kosher salt
• 1/2 teaspoon freshly ground
black pepper
• 2 pounds cooked shrimp, peeled,
tails removed and diced
• 2 celery stalks, finely diced
• 1 tablespoon minced chives
• 1 tomato, sliced
• 6 slices bacon, cooked until crispy
• Bibb lettuce
Preparation
In a large bowl, mix the lemon juice, mayonnaise, vinegar, mustard,
sugar, salt and pepper. Stir in the shrimp, celery and chives.
Split 6 rolls in half and layer 1 tomato slice on each roll bottom. Top
each with a scoop of the shrimp mixture, 1 slice of bacon, 1 lettuce
leaf and roll tops.
For more recipes for dishes your guests will be talking about the next
day, visit saraleebread.com.
Looking Up
NASA’s Juno Mission Detects Jupiter Wave Trains
Based on a Press Release from
JPL, Provided by Bob Eklund
Massive structures of moving air that appear
like waves in Jupiter’s atmosphere were
first detected by NASA’s Voyager missions
during their flybys of the gas-giant world in
1979. The JunoCam camera aboard NASA’s
Juno mission (https://www.nasa.gov/juno,
https://www.missionjuno.swri.edu) to Jupiter
has also imaged the atmosphere. JunoCam
data has detected atmospheric wave trains,
towering atmospheric structures that trail one
after the other as they roam the planet, with
most concentrated near Jupiter’s equator.
The JunoCam imager has resolved smaller
distances between individual wave crests in
these trains than ever seen before. This research
provides valuable information on both
the dynamics of Jupiter’s atmosphere and its
structure in the regions underneath the waves.
“JunoCam has counted more distinct wave
trains than any other spacecraft mission since
Voyager,” said Glenn Orton, a Juno scientist
from NASA’s Jet Propulsion Laboratory in
Pasadena, California. “The trains, which
consist of as few as two waves and as
many as several dozen, can have a distance
between crests as small as about 40 miles
and as large as about 760 miles The shadow
of the wave structure in one image allowed
us to estimate the height of one wave to be
about 6 miles high.”
Most of the waves are seen in elongated
wave trains, spread out in an east-west direction,
with wave crests that are perpendicular
to the orientation of the train. Other fronts
in similar wave trains tilt significantly with
respect to the orientation of the wave train,
and still other wave trains follow slanted or
meandering paths.
“The waves can appear close to other Jovian
atmospheric features, near vortices or along
flow lines, and others exhibit no relationship
with anything nearby,” said Orton. “Some wave
trains appear as if they are converging, and
others appear to be overlapping, possibly at
two different atmospheric levels. In one case,
Three waves can be seen in this excerpt of a JunoCam image taken on Feb. 2, 2017, during Juno’s fourth flyby of Jupiter. The region
imaged in this picture is part of the visibly dark band just north of Jupiter’s equator known as the North Equatorial Belt. Image credit:
NASA/JPL-Caltech/SwRI/MSSS/JunoCam.
wave fronts appear to be radiating outward
from the center of a cyclone.”
Although analysis is ongoing, most waves
are expected to be atmospheric gravity
waves—up and-down ripples that form in
the atmosphere above something that disturbs
air flow, such as a thunderstorm updraft,
disruptions of flow around other features, or
from some other disturbance that JunoCam
does not detect.
The JunoCam instrument is uniquely qualified
to make such a discovery. JunoCam is
a color, visible-light camera which offers a
wide-angle field of view designed to capture
remarkable pictures of Jupiter’s poles and
cloud tops. As Juno’s eyes, it helps provide
context for the spacecraft’s other instruments.
JunoCam was included on the spacecraft
primarily for public engagement purposes,
although its images also are helpful to the
science team.
Juno launched on Aug. 5, 2011, from
Cape Canaveral, Florida, and arrived in orbit
around Jupiter on July 4, 2016. To date, it
has completed 15 science passes over Jupiter.
Juno’s 16th science pass will be on Oct. 29.
During these flybys, Juno is probing beneath
the obscuring cloud cover of Jupiter and
studying its auroras to learn more about the
planet’s origins, structure, atmosphere and
magnetosphere. •
“Jupiter, a world far larger than Earth, is so warm that it currently
radiates more internal heat than it receives from the Sun.”
– Seth Shostak