There are also two golden ticket entries given to the winners of the Group 1 Futurity Stakes (1400m) and Group 2 Blamey Stakes (2000m) should they not already be one of the Top 10 vote-getters. The other positions in the weight-for-age event are filled by Wildcard horses chosen by Racing Victoria. Aussie and Kiwi punters get to vote on their favourite eligible milers, selecting 10 of the now expanded 15 runners in The All-Star Mile field. The All-Star Mile is the only Australian race where members of the public help to choose the final field of horses. The All-Star Mile race returned to Flemington in 2022 and ran the weekend after ‘Super Saturday’ at the track with the favourite Zaaki saluting for the puntes. The 2020 The All-Star Mile moved from Flemington to Caulfield Racecourse and saw the Perth-trained stablemates Regal Power (1st) and Superstorm (2nd) run the quinella.įor 2021 the third edition of The All-Star Mile was conducted at The Valley and won by New South Wales’ visitor Mugatoo, winner of the previous spring’s Group 3 Newcastle Gold Cup. In 2022 the event was officially known as The Seppelt Wines All-Star Mile.įeaturing a prize pool of $5 million, the Special Condition race will rotate year-to-year across all three major Victorian tracks with the inaugural edition taking place in 2019 at Flemington Racecourse and won by that year’s Australian Guineas winning filly Mystic Journey. The GRSI can also provide an independent assessment of DEMO DT fusion power and T burning.Ladbrokes Tip: The Australian Guineas is a good form race to follow for any three-year-old The All-Star Mile contestantsĭesigned in 2018 for middle distance horses, The All-Star Mile is a special conditions race held during the Melbourne Autumn Racing Carnival. They are designed to operate at high count rate although GRSI geometry constraints severely impact on this feature.

The GRSI detector is based on commercial LaBr 3(Ce) inorganic scintillating crystal coupled with a photomultiplier tube or a silicon photomultiplier. Among these, the choice of the collimator diameters at the back side of the neutron detector box up to the GRSI detector, the use of LiH neutron attenuators in front of the GRSI detectors, the GRSI detector material and shielding. For these reasons, only few GRSI parameters can be independently selected to optimize its performance. GRSI features long collimators which diameters are constrained by the neutron flux at the neutron detectors of the Radial Neutron Camera (RNC) system placed in front, which are key to control DEMO DT plasma position. The GRSI design is based on the investigation of the reaction cross sections, on the calculations performed with GENESIS and MCNP simulation codes and on the physics and geometry constrains of the integrated instrument. Due to DEMO tokamak design constraints, the gamma and neutron diagnostics are integrated, both featuring multi-line of sight (camera type), viewing DEMO plasma radially with vertical (12) and horizontal (13) viewing lines to diagnose the γ and neutron emission from the DT plasma poloidal section.

The reaction of interest for this Gamma-Ray Spectrometer Instrument (GRSI) consists of D(T, γ) 5He with the emission of 16.63 MeV γ rays. This work describes the progress of the conceptual study of the gamma-ray diagnostic for DEMO reactor performed during the first Work-Package contract 2015–2020. Among the suite of sensors, an integrated neutron and gamma-ray diagnostic system is also studied to verify its capability and performance in detecting possible DEMO plasma position variations and contribute to the feedback system in maintaining DEMO DT plasma in stable conditions.

The future DEMO tokamak will be equipped with a suite of diagnostics which will operate as sensors to monitor and control the position and operation parameters of DT plasmas.

Star stable codes 2022 january