On 2017-10-15 03:28 PM, Steve Allen wrote:
On Sun 2017-10-15T18:59:31+0000 Michael.Deckers via LEAPSECS hath writ:
  Thank you for these interesting primary sources!
The more I reflect on this the more I realize that Nicolas Stoyko
attended and took notes on many of the astronomy/time/radio meetings
during the 1950s and 1960s.  Lots of the history of who said what when
is in the opening sections of issues of Bulletin Horaire, and detailed
in a way that is not typically found in the official proceedings.
Yes. These references are valuable for the insight they give to the thinking at the time. Thanks.
The 1955 meetings are interesting because atomic time was a thing,
but atomic timescales were not yet a thing anyone had done, and
Ephemeris Time was a thing that a few people had done.
So in all those discussions it is clear that Universal Time is
unquestionably understood to be a measure of earth rotation.

I agree.

The slowing of Earth rotation was suspected early, including by Simon Newcomb They did not have confidence in the reasons for this, and certainly not accurate enough observation nor constant frequency to include it in the Tables of the Sun.

On the possible variability of the Earth's axial rotation, as investigated by Mr. Glasenapp- Simon Newcomb
http://www.ajsonline.org/content/s3-8/45/161.extract#

The references you cite suggest they still expected UT2 could somehow be made to be a uniform scale. Not until atomic time and timescales are established does it become undeniable the Earth rotation was slowing.

It seems the critical development was Essen and Markowitz's determination of the length of the atomic second with respect to Ephemeris Time, completed in 1958. Those efforts are explained in detail by Leschiutta:

The definition of the ‘atomic’ second, Sigfrido Leschiutta
http://geodesy.unr.edu/hanspeterplag/library/geodesy/time/met5_3_S03.pdf

The numbers they'd found were to "stick", resulting in the definition of the SI atomic second and leading to the atomic timescales, eventually to TAI.

Through the early 1960s the many atomic clocks were "coordinated", giving rise to coordinated atomic timescales and the small sub-second frequency and step adjustments required to keep atomic time is step with solar time, as we see in the historical Leap Seconds record.

I find this article by L. Essen most informative of the situation in timescales in 1968, and gives a good summary of how they'd gotten there:

Time Scales, L. ESSEN
Metrologia, Vol.4 , No.4, 1968
http://www.leapsecond.com/history/1968-Metrologia-v4-n4-Essen.pdf

The predisposition toward a single disseminated atomic timescale seems to have taken hold, as he states:

"It would of course be possible to use separate and independent scales of atomic and astronomical time but this possibility already seems to have been rejected, and rightly so in my view, since it would lead to confusion and duplication of effort."

And he concludes with his suggestion for 1s adjustments, which would emerge as "Leap Seconds":

"If it is necessary the minute markers should be moved by 1s at a prearranged date if the deviation between AT and UT2 exceeds 0.5s."

In 1971 J. McA. Steele gives a good explanation of Leap Seconds as they were to be implemented, including an appendix showing the CCIR approved Recommendation 460.

THE IMPROVED UTC SYSTEM TO BE INTRODUCED ON I JANUARY 1972
by J. McA. Steele, August 1971,
https://journals.lib.unb.ca/index.php/ihr/article/viewFile/23857/27642

Barnes gives an excellent summary of the timescales in 1973:

BASIC CONCEPTS OF PRECISE TIME AND FREQUENCY, Barnes, 1973
http://tf.boulder.nist.gov/general/pdf/1593.pdf

I observe -

The development of atomic clocks and timescales had confirmed a new physical phenomenon; constant frequency time by atomic science. The new systems increased accuracy by at least three orders of magnitude over earlier clocks. This, together with improve astronomy, made it possible for the first time to quantify the discrepancies between uniform constant frequency and astronomical time, clearly revealing the Earth's unpredictably slowing rotation.

Thus there are two physical phenomenon, atomic time, and astronomical time, obviously demanding two timescales. But two timescales was seen as difficult and there was a question of priority; which was to be the *reference*? It could really have been done either way; atomic time defining "seconds" (as TAI has become) with astronomical time defined with respect to atomic time (as UTC and UT1 have become), or other way round; astronomical time defining "seconds" ("solar seconds"?) with atomic time defined with respect to astronomical time. Atomic time won that discussion.

UTC is obviously and intentionally an approximation of mean solar time, a compromise between the uninterrupted incrementing TAI SI seconds counting method and the Gregorian YMDhms counting method modified with the Leap Second (23:59:60) to define the boundaries between days. This has left us with the incommensurability between UTC and the classical Gregorian calendar, local time-of-day (conventional clocks), and computer/electronic implementations of Gregorian, local time, and time-of-day.

Speaking of meetings, ITU-R WP7A meets in 10 days and looks likely to
discuss leap seconds.

There continues to be debate and focus on retaining a single timescale and yet this was never actually the case. UTC is really two timescales, (an abstract form of) TAI, together with an approximation of mean solar time via the Leap Seconds modification of the Gregorian counting algorithm. Further, Rec 460 also specifies 1/10th second resolution DUT1, and the radio time signals disseminate this signal too. So, that's really *three* timescales.

Proposed solutions to the UTC v.s. "computer time" problem have focused on delaying the adjustments or, most prominently, simply eliminating Leap Seconds. I think these sorts of solutions will meet the same fate they have in the past, that is, "no action", because it is difficult or impossible to substantially change any standard or protocol that has gained wide acceptance, and UTC might be the most widely used standard of all time. The exception might be the pure Gregorian calendar itself, and therein lies the difficulty; two very widely used timekeeping standards that are incommensurate.

The "smeared" time dissemination services (Google smear, etc) are used to eliminate the Leap Second from the receiver's view of the timescale, restoring a 86400-second-day to the classical Gregorian algorithm. Those methods focus on smearing the 24 or 12 hour periods surrounding the Leap Second. Unfortunately they do not match one another and introduce a rather extreme frequency shift between TAI/UTC and the resulting "Leap-Second-free" timescales on Leap Second days.

I feel UT1 does not receive the attention it deserves. In this context UT1 might be used to fix UTC v.s. "computer time" conundrum by supplying the information to more faithfully and gradually distribute the "smeared" frequency shifts between successive Leap Seconds, retaining traceability to UTC. I think the IERS already produces the raw information in Bulletin D (DUT1) on which an approach like that could be based.

I hope the participants of ITU-R WP7A and contributing organizations might consider redirecting their efforts from seeking to eliminate Leap Seconds to a more robust technical approach that recognizes the need for more than one timescale.

-Brooks


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