NUGGET INDEX FOR 2001

	010105: Motions of coronal-hole boundaries I. Supergranulation In this nugget, we expected to find that the boundaries of the coronal hole would flutter like a Kansas curtain in a thunderstorm, as a consequence of the solar surface motions we call supergranulation. On first look, that may not be the case.
	010112: "Starburst" Images and Scattering Research This week the SXT scientists are gathered for a small workshop dedicated to the subject of this nugget, which is another of our series on how the SXT instrument works. We have to understand all the nitty-gritty details of the instrument before we can be confident about what is real, and what is not, in our data.
	010119: A Flare in an Almost-Anemone When a solar active region emerges in a coronal hole, the new active region may not appear to have any coronal connections to other regions. We call this an "anemone" region, after the windflower. It's noteworthy that the tiny little flare that occurred in this region is more than twice the diameter of Earth!
	010126: A coronal conveyor belt? Normally we write these Yohkoh science nuggets based on interesting phenomena that we spot for the first time in the SXT data. Sometimes we miss something, and in this case, it's what the authors of a published paper describe as the conveyance of energy from one solar active region to another.
	010202: A dark 'S' erupted! Bright 'S' shapes (sigmoids) are popular among solar physicists, especially those who study flares and CMEs. However, the 'S' here is invisible to SXT. A gorgeous dark 'S' shape appeared in SoHO/EIT images and produced a spectacular Coronal Mass Ejection.
	010209: A most peculiar high-energy event Normally we write these Yohkoh science nuggets mostly about coronal soft X-ray sources. In this Nugget we talk about events that emit hard X-rays, gamma-rays, and copious "solar cosmic rays" -- which make the topics that are our bread and butter seem rather flacid.
	010216: A two-sided jet 1,000,000 km long Soft X-ray "jets" were one of the truly new discoveries of Yohkoh/SXT, apparently one that was not anticipated by the NASA Skylab mission 30 years ago. Here we report a huge bi-directional jet that spread out across the solar surface, with a beautiful structure.
	010223: Two-stage dimming Coronal dimming, seen in soft X-rays, should rightly be regarded as one of Yohkoh's major discoveries. This is one of those cases where a coronal disturbance does not focus entirely down to a compact origin (eg a major impulsive flare); instead, there are distinctly global effects.
	010302: Temperature of active region loops In order to understand how the solar corona is heated, the distribution of temperature along a typical X-ray loop is essential information. To get this, you take the ratio of two images in different filters (with slightly different temperature sensitivities), and the ratio directly gives you a temperature.
	010309: A CME and an impulsive flare This week we have had four M-class flares after several weeks of their absence. One of them was very well observed by SXT, and showed many of the fascinating optical, X-ray and radio phenomena that are associated with flares and Coronal Mass Ejections.
	010316: Twin-dimming event of 28 February 2001 Coronal dimming in X-rays and EUV is often discussed in the context of Coronal Mass Ejections (CMEs). Are these dimmings the footpoints of a large magnetic flux rope, which in turn are the central part of the CME?
	010323: "Magnificent cusp", now analyzed We report a success story here: an item we reported in a nugget entitled "A magnificent cusp" two years ago has now been analyzed and published. Now what do we need? More theory!
	010330: What an aurora! Spectacular auroras were seen around the world on March 31, 2001. What happened on the Sun that caused all this hullabaloo? A great big sunspot, a major X-ray flare, and an Earth-directed CME!
	010406: The most powerful solar flare in decades! We missed the fun part of this event, as often happens, so we need another one, preferably one jointly observed with HESSI). Huge events show us more of the things we like to study.
	010413: A beautifully observed major flare Yohkoh was flying through clear sunshine at the time of the flare, leading to great observations. It's becoming clearer and clearer that geometrical re-formation of the coronal magnetic field plays a decisive role in all kinds of phenomena.
	010420: Energetic particles from the far side of the Sun This event is interesting because it shows that a far-side event can have effects at 1 AU due to a shock wave that has a wide longitudinal ecent. It also gives us a chance to think more seriously about the 3-D nature of Coronal Mass Ejections.
	010427: A transient coronal hole Today let's take a break and pick up a little-discussed subject: the nature of "transient coronal holes." The inference here is that magnetic reconnection may not be such an energetic process, and may be dictated more by global coronal conditions than by local physics.
	010504: Hard x-ray ejection: a work in progress This week many other nice things happened on the Sun, but the April 18 event has obsessively preoccupied attention. Why is this? We show some of the work in progress and comment here on why we have dropped everything to pursue it.
	010511: Sigmoid alert and eruptive flares When is an eruption not an eruption? When you call a sigmoid alert! Last week we executed our carefully-laid plans for an observing campaign, based upon the recognition of a new "sigmoid" coronal structure in our images.
	010518: Cleverly-Designed Image Buffers This week let's turn the spotlight backstage and look the instrumentation of the Yohkoh Soft X-ray Telescope, SXT. In this nugget we discuss how the SXT takes various kinds of images of the Sun and sends them to us on the ground.
	010525: Two kinds of CMEs There tend to be two kinds of CMEs -- fast ones, associated with solar flares, and slow ones, associated with the eruption of filaments. "Halo" CMEs -- directed toward or away from Earth -- are of unique importance. How do fast and slow CMEs show up in such events?
	010601: Hard-soft-hard As we get closer to the launch of HESSI (it almost happened this week!), naturally our thoughts turn to the high-energy aspects of solar flares. Solar "hard" X-rays and gamma rays give us quite direct views of these phenomena, compared to the "soft" X-ray emission that the Yohkoh Soft X-Ray Telescope (SXT) images.
	010608: Predicting the Coronal Structure During the Upcoming Total Solar Eclipse The first total solar eclipse of this millennium will be seen on 21st June, 2001, along a path crossing southern Africa through Madagascar. For scientists planning observations, it is helpful to know the global structure of the corona in advance -- but how?.
	010615: All Loops, All the Time When we talk about "coronal loops" in Yohkoh SXT observations, we mean long, slender structures that are seen in the corona. These loops act like hoses, channeling squirts of solar gas driven by heating or cooling.
	010622: How smooth is the Sun? Comparatively speaking, the Sun's surface (photosphere) is really smooth. The thickness of the solar atmosphere is about 0.02% of the solar radius. This corresponds to a 2-mil tolerance on a ten-inch part, in machinist's parlance, not a bad job.
	010629: Where are Coronal Loops Heated? Coronal heating is one of the Big Questions of solar physics. Simply put, this is because understanding how the energy gets transported to the upper atmosphere and deposited there is crucial to figuring out such fundamental things as how the solar wind is accelerated, and why coronal loops are hot.
	010706: Breaking Records -- It's all about Latitude! This week the Sun is showing us a pair of active regions that is unusually far from the equator. Finding the limits of size and latitudinal extent of active regions and CMEs helps us to put constraints on theories of the Sun's magnetic fields.
	010713: Bastille Day throughout history This nugget is nothing more than a transparent ruse by which we get to show you more pretty pictures of solar events that took place on July 14, 2000 (the French Bastille Day). The author's tongue is squarely in his cheek!
	010720: Three-part harmony All you tenors, altos, basses, sopranos, baritones and so forth: this science nugget has nothing to do with music theory. Instead we point out some nice three-part features of coronal mass ejections (CMEs), which are among the most spectacular and beautiful of solar phenomena.
	010727: A solar "Island Universe" The romantic-sounding title of this nugget echoes astronomers' celebrated Shapley-Curtis debates regarding the nature of nebulae. The somewhat farfetched analogy here is suggested by an "island universe" of magnetism on the Sun, seen via the Yohkoh Soft X-Ray Telescope.
	010803: Magnetic collapse and a flare A solar flare consists of an extravagant collection of energetic phenomena - radiation, particle acceleration, expansion, coronal mass ejection, etc. This lavish display needs a source of energy, and this week two SXT scientists think they've found an example that shows that it's extracted from the Sun's magnetic field.
	010810: A gentle giant During a recent period, the sun showed dramatic variability in its coronal structure, but very little variability in its overall X-ray brightness. The huge region that accounted for much of the restructuring is the gentle giant named in the title of this nugget.
	010817: Yohkoh observations of X-class flares Whenever a big (X-class) flare occurs, we are pleased. Such big flares are likely to be observed by many instruments covering a wide wavelength range, and thorough analysis of these data has the potential to give us an important insight into the mechanism(s) that account for these spectacular events.
	010824: Reverberations of April 7, 1997 Sometimes the initial look at a given phenomenon doesn't reveal all of its subtleties. It is nice to see the information accumulating, and this nugget reviews several pieces of work on one of the first really nice flare/CME events of the current solar maximum: April 7, 1997.
	010831: Millimeter waves, white light, and gamma rays The X-class flare of August 25, 2001 had a huge radio flux at short wavelengths. Here is a chance for us to write a nugget showing how all parts of the solar spectrum do things simultaneously in such an event.
	010907: Three X-ray global waves Large-scale (global) coronal waves are launched by yet-mysterious processes in the heart of a solar flare. We now believe that these are probably akin to bow waves driven ahead of CMEs rather than free-running "blast waves" of the sort seen in the corona.
	010914: Cusps Within Cusps We love cusps. There have been several Nuggets dedicated to them (see here ) and several tens mentioning them. We have had Magnificent cusps and Cusps upon Cusps . The Sun continues to surprise us by its ingenuity, and in this Nugget we discuss cusps within cusps, prompted by a very nice example seen this week.
	010921: One Week in the Life of a Sigmoid This week we go back to a set of observations which were made in August of 1999, as part of `Whole Sun Month 3', where, jointly with many other instruments, SXT followed an active region for a week as it crossed the solar disk. Our observations allowed us to see how the region behaved over many days.
	010928: Czech hard X-rays fit beautifully! This is our first opportunity to intercompare Yohkoh data with hard X-ray photometry from the new Czech-built Hard X-ray Spectrometer (HXRS for short). We're pleased to report that the HXRS and Yohkoh data fit well together and can be analyzed.
	011005: Spiny arcades repeat Yohkoh has seen multiple spiny arcades this week. A pointy coronal streamer is a often called a "helmet streamer", but following this analogy a spiny arcade would be more like a whole platoon of Prussian soldiers wearing helmets with spikes.